The Physical Properties of the Groups of Galaxies
Galaxy groups consist of a few tens of galaxies bound in a common gravitational potential and contain a significant fraction of the overall universal baryon budget. Therefore, they are key to our understanding of how the bulk of matter in the Universe accretes and forms hierarchical structures and h...
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| Year of Publication: | 2021 |
| Language: | English |
| Physical Description: | 1 electronic resource (250 p.) |
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(CKB)5400000000044690 (oapen)https://directory.doabooks.org/handle/20.500.12854/76813 (EXLCZ)995400000000044690 |
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Lovisari, Lorenzo edt The Physical Properties of the Groups of Galaxies Basel, Switzerland MDPI - Multidisciplinary Digital Publishing Institute 2021 1 electronic resource (250 p.) text txt rdacontent computer c rdamedia online resource cr rdacarrier Galaxy groups consist of a few tens of galaxies bound in a common gravitational potential and contain a significant fraction of the overall universal baryon budget. Therefore, they are key to our understanding of how the bulk of matter in the Universe accretes and forms hierarchical structures and how different sources of feedback affect their gravitational collapse. However, despite their crucial role in cosmic structure formation and evolution, galaxy groups have received less attention compared to massive clusters. This is perhaps in part due to their rarity in being observed and properly characterized. With the advent of eROSITA, many thousands of galaxy groups will be detected by X-ray, complementing optical and SZ coverage. In this Special Issue we collected and organized the latest developments in our understanding of these systems and present future prospects from both observational and theoretical points of view. English Research & information: general bicssc fossil galaxy groups galaxy clusters galaxy groups X-ray and optical observations hydrodynamical simulations intragroup medium/plasma active galactic nuclei black holes elliptical galaxies active nuclei X-ray observations hydrodynamical and cosmological simulations galaxies:abundances galaxies:clusters:intracluster medium X-rays:galaxies galaxy surveys UV observations cosmological parameters 3-0365-1773-1 3-0365-1774-X Ettori, Stefano edt Lovisari, Lorenzo oth Ettori, Stefano oth |
| language |
English |
| format |
eBook |
| author2 |
Ettori, Stefano Lovisari, Lorenzo Ettori, Stefano |
| author_facet |
Ettori, Stefano Lovisari, Lorenzo Ettori, Stefano |
| author2_variant |
l l ll s e se |
| author2_role |
HerausgeberIn Sonstige Sonstige |
| title |
The Physical Properties of the Groups of Galaxies |
| spellingShingle |
The Physical Properties of the Groups of Galaxies |
| title_full |
The Physical Properties of the Groups of Galaxies |
| title_fullStr |
The Physical Properties of the Groups of Galaxies |
| title_full_unstemmed |
The Physical Properties of the Groups of Galaxies |
| title_auth |
The Physical Properties of the Groups of Galaxies |
| title_new |
The Physical Properties of the Groups of Galaxies |
| title_sort |
the physical properties of the groups of galaxies |
| publisher |
MDPI - Multidisciplinary Digital Publishing Institute |
| publishDate |
2021 |
| physical |
1 electronic resource (250 p.) |
| isbn |
3-0365-1773-1 3-0365-1774-X |
| illustrated |
Not Illustrated |
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AT lovisarilorenzo thephysicalpropertiesofthegroupsofgalaxies AT ettoristefano thephysicalpropertiesofthegroupsofgalaxies |
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(CKB)5400000000044690 (oapen)https://directory.doabooks.org/handle/20.500.12854/76813 (EXLCZ)995400000000044690 |
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The Physical Properties of the Groups of Galaxies |
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