The Central Dark Matter Fraction of Massive Early-Type Galaxies
Dark matter (DM) is predicted to be the dominant mass component in galaxies. In the central region of early-type galaxies it is expected to account for a large amount of the total mass, although the stellar mass should still represent the majority of the mass budget, depending on the stellar initial...
| Main Authors: | , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Frontiers Media S.A.
2022-01-01
|
| Series: | Frontiers in Astronomy and Space Sciences |
| Subjects: | |
| Online Access: | https://www.frontiersin.org/articles/10.3389/fspas.2021.704419/full |
| _version_ | 1818332522351689728 |
|---|---|
| author | C. Tortora N. R. Napolitano N. R. Napolitano |
| author_facet | C. Tortora N. R. Napolitano N. R. Napolitano |
| author_sort | C. Tortora |
| collection | DOAJ |
| description | Dark matter (DM) is predicted to be the dominant mass component in galaxies. In the central region of early-type galaxies it is expected to account for a large amount of the total mass, although the stellar mass should still represent the majority of the mass budget, depending on the stellar initial mass function (IMF). We discuss latest results on the DM fraction and mean DM density for local galaxies and explore their evolution with redshifts in the last 8 Gyr of the cosmic history. We compare these results with expectations from the ΛCDM model and discuss the role of the IMF and galaxy model through the central total mass density slope. We finally present future perspectives offered by next-generation instruments/surveys (Rubin/LSST, Euclid, CSST, WEAVE, 4MOST, and DESI), which will provide the unique chance to measure the DM evolution with time for an unprecedented number of galaxies and constrain their evolutionary scenario. |
| first_indexed | 2024-12-13T13:37:05Z |
| format | Article |
| id | doaj.art-3efc6cd12b5c418f8685ca245d93e199 |
| institution | Directory Open Access Journal |
| issn | 2296-987X |
| language | English |
| last_indexed | 2024-12-13T13:37:05Z |
| publishDate | 2022-01-01 |
| publisher | Frontiers Media S.A. |
| record_format | Article |
| series | Frontiers in Astronomy and Space Sciences |
| spelling | doaj.art-3efc6cd12b5c418f8685ca245d93e1992022-12-21T23:43:43ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2022-01-01810.3389/fspas.2021.704419704419The Central Dark Matter Fraction of Massive Early-Type GalaxiesC. Tortora0N. R. Napolitano1N. R. Napolitano2School of Physics and Astronomy, Sun Yat-sen University Zhuhai Campus, Zhuhai, ChinaSchool of Physics and Astronomy, Sun Yat-sen University Zhuhai Campus, Zhuhai, ChinaINAF—Osservatorio Astronomico di Capodimonte, Napoli, ItalyDark matter (DM) is predicted to be the dominant mass component in galaxies. In the central region of early-type galaxies it is expected to account for a large amount of the total mass, although the stellar mass should still represent the majority of the mass budget, depending on the stellar initial mass function (IMF). We discuss latest results on the DM fraction and mean DM density for local galaxies and explore their evolution with redshifts in the last 8 Gyr of the cosmic history. We compare these results with expectations from the ΛCDM model and discuss the role of the IMF and galaxy model through the central total mass density slope. We finally present future perspectives offered by next-generation instruments/surveys (Rubin/LSST, Euclid, CSST, WEAVE, 4MOST, and DESI), which will provide the unique chance to measure the DM evolution with time for an unprecedented number of galaxies and constrain their evolutionary scenario.https://www.frontiersin.org/articles/10.3389/fspas.2021.704419/fulldark matter - galaxiesgalaxies: formation -galaxies: evolution -galaxies: ellipticalsurveys - galaxies |
| spellingShingle | C. Tortora N. R. Napolitano N. R. Napolitano The Central Dark Matter Fraction of Massive Early-Type Galaxies Frontiers in Astronomy and Space Sciences dark matter - galaxies galaxies: formation - galaxies: evolution - galaxies: elliptical surveys - galaxies |
| title | The Central Dark Matter Fraction of Massive Early-Type Galaxies |
| title_full | The Central Dark Matter Fraction of Massive Early-Type Galaxies |
| title_fullStr | The Central Dark Matter Fraction of Massive Early-Type Galaxies |
| title_full_unstemmed | The Central Dark Matter Fraction of Massive Early-Type Galaxies |
| title_short | The Central Dark Matter Fraction of Massive Early-Type Galaxies |
| title_sort | central dark matter fraction of massive early type galaxies |
| topic | dark matter - galaxies galaxies: formation - galaxies: evolution - galaxies: elliptical surveys - galaxies |
| url | https://www.frontiersin.org/articles/10.3389/fspas.2021.704419/full |
| work_keys_str_mv | AT ctortora thecentraldarkmatterfractionofmassiveearlytypegalaxies AT nrnapolitano thecentraldarkmatterfractionofmassiveearlytypegalaxies AT nrnapolitano thecentraldarkmatterfractionofmassiveearlytypegalaxies AT ctortora centraldarkmatterfractionofmassiveearlytypegalaxies AT nrnapolitano centraldarkmatterfractionofmassiveearlytypegalaxies AT nrnapolitano centraldarkmatterfractionofmassiveearlytypegalaxies |