High-Energy Astrophysics / / Fulvio Melia.

High-energy astrophysics involves the study of exceedingly dynamic and energetic phenomena occurring near the most extreme celestial objects known to exist, such as black holes, neutron stars, white dwarfs, and supernova remnants. High-Energy Astrophysics provides graduate and advanced undergraduate...

Full description

Saved in:
Bibliographic Details
Superior document:Title is part of eBook package: De Gruyter Princeton University Press eBook-Package Backlist 2000-2013
VerfasserIn:
Place / Publishing House:Princeton, NJ : : Princeton University Press, , [2021]
©2009
Year of Publication:2021
Language:English
Series:Princeton Series in Astrophysics ; 14
Online Access:
Physical Description:1 online resource (392 p.) :; 26 color illus. 52 halftones. 59 line illus.
Tags: Add Tag
No Tags, Be the first to tag this record!
id 9781400833375
ctrlnum (DE-B1597)613961
(OCoLC)1291506742
collection bib_alma
record_format marc
spelling Melia, Fulvio, author. aut http://id.loc.gov/vocabulary/relators/aut
High-Energy Astrophysics / Fulvio Melia.
Princeton, NJ : Princeton University Press, [2021]
©2009
1 online resource (392 p.) : 26 color illus. 52 halftones. 59 line illus.
text txt rdacontent
computer c rdamedia
online resource cr rdacarrier
text file PDF rda
Princeton Series in Astrophysics ; 14
Frontmatter -- Contents -- Preface -- Chapter 1. Introduction and Motivation -- Chapter 2. The High-Energy Sky -- Chapter 3. Relativity -- Chapter 4. Particle Acceleration -- Chapter 5. Radiative Processes -- Chapter 6. Accretion of Plasma -- Chapter 7. Accretion Disk Theory -- Chapter 8. Thick Accretion Disks -- Chapter 9. Pulsing Sources -- Chapter 10. Black Holes in Binaries -- Chapter 11. Bursting Stars -- Chapter 12. Supermassive Black Holes -- Chapter 13. The High-Energy Background -- Bibliography -- Index
restricted access http://purl.org/coar/access_right/c_16ec online access with authorization star
High-energy astrophysics involves the study of exceedingly dynamic and energetic phenomena occurring near the most extreme celestial objects known to exist, such as black holes, neutron stars, white dwarfs, and supernova remnants. High-Energy Astrophysics provides graduate and advanced undergraduate students with the most complete, self-contained introduction to the subject available. This textbook covers all the essentials, weaving together the latest theory with the experimental techniques, instrumentation, and observational methods astronomers use to study high-energy radiation from space. Fulvio Melia introduces topics at the forefront of today's research, including relativistic particles, energetic radiation, and accretion disk theory. No other textbook offers such a thorough yet concise treatment of the key aspects of high-energy astrophysics--both theoretical and observational--or delves as deeply into modern detection techniques, satellite systems, and analytical and numerical modeling used by theoreticians. Amply illustrated, High-Energy Astrophysics is also ideal for researchers interested in the application of fundamental physical laws to understand how matter and radiation behave in regions of the universe where physical conditions are most extreme.Uniquely weaves together the theoretical and experimental aspects of this important branch of astronomy Features stunning images of the high-energy sky Fully describes the principal classes of high-energy sources, with an in-depth study of many archetypal objects within them Provides an excellent, self-contained resource for the classroom, written by a preeminent researcher and teacher in the field
Mode of access: Internet via World Wide Web.
In English.
Description based on online resource; title from PDF title page (publisher's Web site, viewed 29. Jun 2022)
Astrophysics.
Nuclear astrophysics.
SCIENCE / Physics / Astrophysics. bisacsh
Acceleration.
Accretion (astrophysics).
Accretion disk.
Active galactic nucleus.
Amplitude.
Angular momentum.
Annihilation.
Apsis.
Arbitrarily large.
BL Lac object.
Bell's theorem.
Binary star.
Black hole.
Boundary layer.
Bremsstrahlung.
Circular orbit.
Classical mechanics.
Classical physics.
Compact star.
Compton Gamma Ray Observatory.
Compton scattering.
Concept.
Conceptual framework.
Conjecture.
Cosmic ray.
Cygnus A.
Cygnus X-1.
Database.
Dissipation.
Doppler effect.
Effective temperature.
Emissivity.
Event horizon.
Four-dimensional space.
Four-vector.
Galactic Center.
Galactic plane.
Galaxy cluster.
Gamma-ray burst.
Gravitational energy.
Initial condition.
Instability.
Interstellar medium.
Intracluster medium.
Luminosity function (astronomy).
Magnetic field.
Massive particle.
Measurement.
Milky Way.
Minute and second of arc.
Molecular cloud.
Molecule.
Neutron star.
Nuclear reaction.
Ontology.
Optical depth.
Orbital period.
Particle physics.
Phenomenon.
Photon.
Physical law.
Physical quantity.
Physicist.
Pierre Auger Observatory.
Pilot wave.
Polytropic process.
Positron.
Power law.
Prediction.
Probability.
Quantity.
Quantum decoherence.
Quantum mechanics.
Quasar.
ROSAT.
Radiative cooling.
Radiative flux.
Roche lobe.
Scattering.
Spaceflight.
Special relativity.
Star.
Supermassive black hole.
Supernova.
Synchrotron.
Temperature.
Theorem.
Theory of relativity.
Theory.
Thin disk.
Time dilation.
Transonic.
Virgo Cluster.
Viscosity.
Wave function.
Wavelength.
White dwarf.
X-ray.
XMM-Newton.
Title is part of eBook package: De Gruyter Princeton University Press eBook-Package Backlist 2000-2013 9783110442502
Title is part of eBook package: De Gruyter Princeton University Press eBook-Package Gap Years 9783110784237
https://doi.org/10.1515/9781400833375?locatt=mode:legacy
https://www.degruyter.com/isbn/9781400833375
Cover https://www.degruyter.com/document/cover/isbn/9781400833375/original
language English
format eBook
author Melia, Fulvio,
Melia, Fulvio,
spellingShingle Melia, Fulvio,
Melia, Fulvio,
High-Energy Astrophysics /
Princeton Series in Astrophysics ;
Frontmatter --
Contents --
Preface --
Chapter 1. Introduction and Motivation --
Chapter 2. The High-Energy Sky --
Chapter 3. Relativity --
Chapter 4. Particle Acceleration --
Chapter 5. Radiative Processes --
Chapter 6. Accretion of Plasma --
Chapter 7. Accretion Disk Theory --
Chapter 8. Thick Accretion Disks --
Chapter 9. Pulsing Sources --
Chapter 10. Black Holes in Binaries --
Chapter 11. Bursting Stars --
Chapter 12. Supermassive Black Holes --
Chapter 13. The High-Energy Background --
Bibliography --
Index
author_facet Melia, Fulvio,
Melia, Fulvio,
author_variant f m fm
f m fm
author_role VerfasserIn
VerfasserIn
author_sort Melia, Fulvio,
title High-Energy Astrophysics /
title_full High-Energy Astrophysics / Fulvio Melia.
title_fullStr High-Energy Astrophysics / Fulvio Melia.
title_full_unstemmed High-Energy Astrophysics / Fulvio Melia.
title_auth High-Energy Astrophysics /
title_alt Frontmatter --
Contents --
Preface --
Chapter 1. Introduction and Motivation --
Chapter 2. The High-Energy Sky --
Chapter 3. Relativity --
Chapter 4. Particle Acceleration --
Chapter 5. Radiative Processes --
Chapter 6. Accretion of Plasma --
Chapter 7. Accretion Disk Theory --
Chapter 8. Thick Accretion Disks --
Chapter 9. Pulsing Sources --
Chapter 10. Black Holes in Binaries --
Chapter 11. Bursting Stars --
Chapter 12. Supermassive Black Holes --
Chapter 13. The High-Energy Background --
Bibliography --
Index
title_new High-Energy Astrophysics /
title_sort high-energy astrophysics /
series Princeton Series in Astrophysics ;
series2 Princeton Series in Astrophysics ;
publisher Princeton University Press,
publishDate 2021
physical 1 online resource (392 p.) : 26 color illus. 52 halftones. 59 line illus.
contents Frontmatter --
Contents --
Preface --
Chapter 1. Introduction and Motivation --
Chapter 2. The High-Energy Sky --
Chapter 3. Relativity --
Chapter 4. Particle Acceleration --
Chapter 5. Radiative Processes --
Chapter 6. Accretion of Plasma --
Chapter 7. Accretion Disk Theory --
Chapter 8. Thick Accretion Disks --
Chapter 9. Pulsing Sources --
Chapter 10. Black Holes in Binaries --
Chapter 11. Bursting Stars --
Chapter 12. Supermassive Black Holes --
Chapter 13. The High-Energy Background --
Bibliography --
Index
isbn 9781400833375
9783110442502
9783110784237
url https://doi.org/10.1515/9781400833375?locatt=mode:legacy
https://www.degruyter.com/isbn/9781400833375
https://www.degruyter.com/document/cover/isbn/9781400833375/original
illustrated Illustrated
dewey-hundreds 500 - Science
dewey-tens 520 - Astronomy
dewey-ones 523 - Specific celestial bodies & phenomena
dewey-full 523.01/97
dewey-sort 3523.01 297
dewey-raw 523.01/97
dewey-search 523.01/97
doi_str_mv 10.1515/9781400833375?locatt=mode:legacy
oclc_num 1291506742
work_keys_str_mv AT meliafulvio highenergyastrophysics
status_str n
ids_txt_mv (DE-B1597)613961
(OCoLC)1291506742
carrierType_str_mv cr
hierarchy_parent_title Title is part of eBook package: De Gruyter Princeton University Press eBook-Package Backlist 2000-2013
Title is part of eBook package: De Gruyter Princeton University Press eBook-Package Gap Years
is_hierarchy_title High-Energy Astrophysics /
container_title Title is part of eBook package: De Gruyter Princeton University Press eBook-Package Backlist 2000-2013
_version_ 1770176645336924160
fullrecord <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>07979nam a22018855i 4500</leader><controlfield tag="001">9781400833375</controlfield><controlfield tag="003">DE-B1597</controlfield><controlfield tag="005">20220629043637.0</controlfield><controlfield tag="006">m|||||o||d||||||||</controlfield><controlfield tag="007">cr || ||||||||</controlfield><controlfield tag="008">220629t20212009nju fo d z eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9781400833375</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1515/9781400833375</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-B1597)613961</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1291506742</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-B1597</subfield><subfield code="b">eng</subfield><subfield code="c">DE-B1597</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="044" ind1=" " ind2=" "><subfield code="a">nju</subfield><subfield code="c">US-NJ</subfield></datafield><datafield tag="072" ind1=" " ind2="7"><subfield code="a">SCI005000</subfield><subfield code="2">bisacsh</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">523.01/97</subfield><subfield code="2">22</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Melia, Fulvio, </subfield><subfield code="e">author.</subfield><subfield code="4">aut</subfield><subfield code="4">http://id.loc.gov/vocabulary/relators/aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">High-Energy Astrophysics /</subfield><subfield code="c">Fulvio Melia.</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Princeton, NJ : </subfield><subfield code="b">Princeton University Press, </subfield><subfield code="c">[2021]</subfield></datafield><datafield tag="264" ind1=" " ind2="4"><subfield code="c">©2009</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 online resource (392 p.) :</subfield><subfield code="b">26 color illus. 52 halftones. 59 line illus.</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">computer</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">online resource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="347" ind1=" " ind2=" "><subfield code="a">text file</subfield><subfield code="b">PDF</subfield><subfield code="2">rda</subfield></datafield><datafield tag="490" ind1="0" ind2=" "><subfield code="a">Princeton Series in Astrophysics ;</subfield><subfield code="v">14</subfield></datafield><datafield tag="505" ind1="0" ind2="0"><subfield code="t">Frontmatter -- </subfield><subfield code="t">Contents -- </subfield><subfield code="t">Preface -- </subfield><subfield code="t">Chapter 1. Introduction and Motivation -- </subfield><subfield code="t">Chapter 2. The High-Energy Sky -- </subfield><subfield code="t">Chapter 3. Relativity -- </subfield><subfield code="t">Chapter 4. Particle Acceleration -- </subfield><subfield code="t">Chapter 5. Radiative Processes -- </subfield><subfield code="t">Chapter 6. Accretion of Plasma -- </subfield><subfield code="t">Chapter 7. Accretion Disk Theory -- </subfield><subfield code="t">Chapter 8. Thick Accretion Disks -- </subfield><subfield code="t">Chapter 9. Pulsing Sources -- </subfield><subfield code="t">Chapter 10. Black Holes in Binaries -- </subfield><subfield code="t">Chapter 11. Bursting Stars -- </subfield><subfield code="t">Chapter 12. Supermassive Black Holes -- </subfield><subfield code="t">Chapter 13. The High-Energy Background -- </subfield><subfield code="t">Bibliography -- </subfield><subfield code="t">Index</subfield></datafield><datafield tag="506" ind1="0" ind2=" "><subfield code="a">restricted access</subfield><subfield code="u">http://purl.org/coar/access_right/c_16ec</subfield><subfield code="f">online access with authorization</subfield><subfield code="2">star</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">High-energy astrophysics involves the study of exceedingly dynamic and energetic phenomena occurring near the most extreme celestial objects known to exist, such as black holes, neutron stars, white dwarfs, and supernova remnants. High-Energy Astrophysics provides graduate and advanced undergraduate students with the most complete, self-contained introduction to the subject available. This textbook covers all the essentials, weaving together the latest theory with the experimental techniques, instrumentation, and observational methods astronomers use to study high-energy radiation from space. Fulvio Melia introduces topics at the forefront of today's research, including relativistic particles, energetic radiation, and accretion disk theory. No other textbook offers such a thorough yet concise treatment of the key aspects of high-energy astrophysics--both theoretical and observational--or delves as deeply into modern detection techniques, satellite systems, and analytical and numerical modeling used by theoreticians. Amply illustrated, High-Energy Astrophysics is also ideal for researchers interested in the application of fundamental physical laws to understand how matter and radiation behave in regions of the universe where physical conditions are most extreme.Uniquely weaves together the theoretical and experimental aspects of this important branch of astronomy Features stunning images of the high-energy sky Fully describes the principal classes of high-energy sources, with an in-depth study of many archetypal objects within them Provides an excellent, self-contained resource for the classroom, written by a preeminent researcher and teacher in the field</subfield></datafield><datafield tag="538" ind1=" " ind2=" "><subfield code="a">Mode of access: Internet via World Wide Web.</subfield></datafield><datafield tag="546" ind1=" " ind2=" "><subfield code="a">In English.</subfield></datafield><datafield tag="588" ind1="0" ind2=" "><subfield code="a">Description based on online resource; title from PDF title page (publisher's Web site, viewed 29. Jun 2022)</subfield></datafield><datafield tag="650" ind1=" " ind2="0"><subfield code="a">Astrophysics.</subfield></datafield><datafield tag="650" ind1=" " ind2="0"><subfield code="a">Nuclear astrophysics.</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">SCIENCE / Physics / Astrophysics.</subfield><subfield code="2">bisacsh</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Acceleration.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Accretion (astrophysics).</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Accretion disk.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Active galactic nucleus.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Amplitude.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Angular momentum.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Annihilation.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Apsis.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Arbitrarily large.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Astrophysics.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">BL Lac object.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Bell's theorem.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Binary star.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Black hole.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Boundary layer.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Bremsstrahlung.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Circular orbit.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Classical mechanics.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Classical physics.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Compact star.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Compton Gamma Ray Observatory.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Compton scattering.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Concept.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Conceptual framework.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Conjecture.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Cosmic ray.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Cygnus A.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Cygnus X-1.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Database.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Dissipation.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Doppler effect.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Effective temperature.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Emissivity.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Event horizon.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Four-dimensional space.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Four-vector.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Galactic Center.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Galactic plane.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Galaxy cluster.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Gamma-ray burst.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Gravitational energy.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Initial condition.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Instability.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Interstellar medium.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Intracluster medium.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Luminosity function (astronomy).</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Magnetic field.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Massive particle.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Measurement.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Milky Way.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Minute and second of arc.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Molecular cloud.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Molecule.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Neutron star.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Nuclear reaction.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Ontology.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Optical depth.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Orbital period.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Particle physics.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Phenomenon.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Photon.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Physical law.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Physical quantity.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Physicist.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Pierre Auger Observatory.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Pilot wave.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Polytropic process.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Positron.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Power law.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Prediction.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Probability.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Quantity.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Quantum decoherence.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Quantum mechanics.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Quasar.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">ROSAT.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Radiative cooling.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Radiative flux.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Roche lobe.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Scattering.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Spaceflight.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Special relativity.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Star.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Supermassive black hole.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Supernova.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Synchrotron.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Temperature.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Theorem.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Theory of relativity.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Theory.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Thin disk.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Time dilation.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Transonic.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Virgo Cluster.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Viscosity.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Wave function.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">Wavelength.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">White dwarf.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">X-ray.</subfield></datafield><datafield tag="653" ind1=" " ind2=" "><subfield code="a">XMM-Newton.</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Title is part of eBook package:</subfield><subfield code="d">De Gruyter</subfield><subfield code="t">Princeton University Press eBook-Package Backlist 2000-2013</subfield><subfield code="z">9783110442502</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Title is part of eBook package:</subfield><subfield code="d">De Gruyter</subfield><subfield code="t">Princeton University Press eBook-Package Gap Years</subfield><subfield code="z">9783110784237</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1515/9781400833375?locatt=mode:legacy</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://www.degruyter.com/isbn/9781400833375</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="3">Cover</subfield><subfield code="u">https://www.degruyter.com/document/cover/isbn/9781400833375/original</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">978-3-11-044250-2 Princeton University Press eBook-Package Backlist 2000-2013</subfield><subfield code="c">2000</subfield><subfield code="d">2013</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">978-3-11-078423-7 Princeton University Press eBook-Package Gap Years</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">EBA_BACKALL</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">EBA_CL_MTPY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">EBA_EBACKALL</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">EBA_EBKALL</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">EBA_ECL_MTPY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">EBA_EEBKALL</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">EBA_ESTMALL</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">EBA_PPALL</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">EBA_STMALL</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV-deGruyter-alles</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">PDA12STME</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">PDA13ENGE</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">PDA18STMEE</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">PDA5EBK</subfield></datafield></record></collection>