Possible Imprints of Cold-mode Accretion on the Present-day Properties of Disk Galaxies Article Swipe
Recent theoretical studies suggest that a significant part of the primordial gas accretes onto forming galaxies as narrow filaments of cold gas without building a shock and experiencing heating. Using a simple model of disk galaxy evolution that combines the growth of dark matter halos predicted by cosmological simulations with a hypothetical form of cold-mode accretion, we investigate how this cold-accretion mode affects the formation process of disk galaxies. It is found that the shock-heating and cold-accretion models produce compatible results for low-mass galaxies owing to the short cooling timescale in such galaxies. However, cold accretion significantly alters the evolution of disk galaxies more massive than the Milky Way and puts observable fingerprints on their present properties. For a galaxy with a virial mass , the scale length of the stellar disk is larger by 41% in the cold-accretion model than in the shock-heating model, with the former model reproducing the steep rise in the size–mass relation observed at the high-mass end. Furthermore, the stellar component of massive galaxies becomes significantly redder (0.66 in u − r at ), and the observed color–mass relation in nearby galaxies is qualitatively reproduced. These results suggest that large disk galaxies with red optical colors may be the product of cold-mode accretion. The essential role of cold accretion is to promote disk formation in the intermediate-evolution phase ( ) by providing the primordial gas having large angular momentum and to terminate late-epoch accretion, quenching star formation and making massive galaxies red.
Related Topics
Concepts
Physics
Astrophysics
Astronomy
Accretion (finance)
Galaxy formation and evolution
Galaxy
Cold dark matter
Peculiar galaxy
Stellar mass
Elliptical galaxy
Star formation
Lenticular galaxy
Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/aaa484
- https://iopscience.iop.org/article/10.3847/1538-4357/aaa484/pdf
- OA Status
- bronze
- Cited By
- 8
- References
- 129
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W2785170507
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W2785170507Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4357/aaa484Digital Object Identifier
- Title
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Possible Imprints of Cold-mode Accretion on the Present-day Properties of Disk GalaxiesWork title
- Type
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articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2018Year of publication
- Publication date
-
2018-01-20Full publication date if available
- Authors
-
Masafumi NoguchiList of authors in order
- Landing page
-
https://doi.org/10.3847/1538-4357/aaa484Publisher landing page
- PDF URL
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https://iopscience.iop.org/article/10.3847/1538-4357/aaa484/pdfDirect link to full text PDF
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YesWhether a free full text is available
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bronzeOpen access status per OpenAlex
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https://iopscience.iop.org/article/10.3847/1538-4357/aaa484/pdfDirect OA link when available
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Physics, Astrophysics, Astronomy, Accretion (finance), Galaxy formation and evolution, Galaxy, Cold dark matter, Peculiar galaxy, Stellar mass, Elliptical galaxy, Star formation, Lenticular galaxyTop concepts (fields/topics) attached by OpenAlex
- Cited by
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8Total citation count in OpenAlex
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2024: 1, 2021: 1, 2020: 3, 2019: 1, 2018: 2Per-year citation counts (last 5 years)
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129Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.is | 71, 133, 188, 215 |
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| abstract_inverted_index.to | 86, 216, 236 |
| abstract_inverted_index.we | 57 |
| abstract_inverted_index.41% | 136 |
| abstract_inverted_index.For | 118 |
| abstract_inverted_index.The | 209 |
| abstract_inverted_index.Way | 109 |
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| abstract_inverted_index.with | 50, 121, 146, 198 |
| abstract_inverted_index.(0.66 | 173 |
| abstract_inverted_index.Milky | 108 |
| abstract_inverted_index.These | 191 |
| abstract_inverted_index.Using | 30 |
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| abstract_inverted_index.colors | 201 |
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| abstract_inverted_index.galaxy | 36, 120 |
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| abstract_inverted_index.angular | 233 |
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| abstract_inverted_index.optical | 200 |
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| abstract_inverted_index.product | 205 |
| abstract_inverted_index.promote | 217 |
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| abstract_inverted_index.Abstract | 0 |
| abstract_inverted_index.However, | 94 |
| abstract_inverted_index.accretes | 13 |
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| abstract_inverted_index.combines | 39 |
| abstract_inverted_index.galaxies | 16, 84, 103, 169, 187, 197, 246 |
| abstract_inverted_index.heating. | 29 |
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| abstract_inverted_index.momentum | 234 |
| abstract_inverted_index.observed | 158, 182 |
| abstract_inverted_index.relation | 157, 184 |
| abstract_inverted_index.accretion | 96, 214 |
| abstract_inverted_index.cold-mode | 55, 207 |
| abstract_inverted_index.component | 166 |
| abstract_inverted_index.essential | 210 |
| abstract_inverted_index.evolution | 37, 100 |
| abstract_inverted_index.filaments | 19 |
| abstract_inverted_index.formation | 65, 219, 242 |
| abstract_inverted_index.galaxies. | 69, 93 |
| abstract_inverted_index.high-mass | 161 |
| abstract_inverted_index.predicted | 46 |
| abstract_inverted_index.providing | 227 |
| abstract_inverted_index.quenching | 240 |
| abstract_inverted_index.terminate | 237 |
| abstract_inverted_index.timescale | 90 |
| abstract_inverted_index.accretion, | 56, 239 |
| abstract_inverted_index.accretion. | 208 |
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| abstract_inverted_index.investigate | 58 |
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| cited_by_percentile_year.min | 89 |
| corresponding_author_ids | https://openalex.org/A5000872706 |
| countries_distinct_count | 1 |
| institutions_distinct_count | 1 |
| corresponding_institution_ids | https://openalex.org/I201537933 |
| citation_normalized_percentile.value | 0.81238229 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |