The shapes and ages of elliptical galaxies
In this paper we investigate the relation between the detailed isophotal shape of elliptical galaxies and the strength of the Hβ absorption in their spectra. We find that discy galaxies have higher Hβ indices. Stellar population synthesis models show that the Hβ line is a good age indicator, hence d...
| Main Authors: | , |
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| Format: | Journal article |
| Language: | English |
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1997
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| _version_ | 1797092523453186048 |
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| author | deJong, R Davies, R |
| author_facet | deJong, R Davies, R |
| author_sort | deJong, R |
| collection | OXFORD |
| description | In this paper we investigate the relation between the detailed isophotal shape of elliptical galaxies and the strength of the Hβ absorption in their spectra. We find that discy galaxies have higher Hβ indices. Stellar population synthesis models show that the Hβ line is a good age indicator, hence discy galaxies tend to have lower mean ages than boxy galaxies. We show that the observed trend can be brought about by a contaminating young population, which we associate with the discy component. This population need only account for a small fraction of the total mass: for example, if a contaminating population of age 2 Gyr is superimposed on an old (12 Gyr) elliptical galaxy, then the observed trend can be explained if it contributes only 10 per cent to the total mass. The size of this effect is consistent with the estimates of disc-to-total light ratios from surface photometry. © 1997 RAS. |
| first_indexed | 2024-03-07T03:47:09Z |
| format | Journal article |
| id | oxford-uuid:bfdeb72f-e24d-44e9-976e-304279d19345 |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-07T03:47:09Z |
| publishDate | 1997 |
| record_format | dspace |
| spelling | oxford-uuid:bfdeb72f-e24d-44e9-976e-304279d193452022-03-27T05:50:40ZThe shapes and ages of elliptical galaxiesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:bfdeb72f-e24d-44e9-976e-304279d19345EnglishSymplectic Elements at Oxford1997deJong, RDavies, RIn this paper we investigate the relation between the detailed isophotal shape of elliptical galaxies and the strength of the Hβ absorption in their spectra. We find that discy galaxies have higher Hβ indices. Stellar population synthesis models show that the Hβ line is a good age indicator, hence discy galaxies tend to have lower mean ages than boxy galaxies. We show that the observed trend can be brought about by a contaminating young population, which we associate with the discy component. This population need only account for a small fraction of the total mass: for example, if a contaminating population of age 2 Gyr is superimposed on an old (12 Gyr) elliptical galaxy, then the observed trend can be explained if it contributes only 10 per cent to the total mass. The size of this effect is consistent with the estimates of disc-to-total light ratios from surface photometry. © 1997 RAS. |
| spellingShingle | deJong, R Davies, R The shapes and ages of elliptical galaxies |
| title | The shapes and ages of elliptical galaxies |
| title_full | The shapes and ages of elliptical galaxies |
| title_fullStr | The shapes and ages of elliptical galaxies |
| title_full_unstemmed | The shapes and ages of elliptical galaxies |
| title_short | The shapes and ages of elliptical galaxies |
| title_sort | shapes and ages of elliptical galaxies |
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