The continuing formation of early-type galaxies: an HI survey
A deep H I survey of nearby early-type galaxies carried out with the Westerbork Radio Synthesis telescope has shown that, contrary to expectation, neutral hydrogen is a significant constituent of the ISM in this type of objects located in low density environment. The studied galaxies are part of a r...
| Váldodahkkit: | , , , , , , , , , |
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| Materiálatiipa: | Conference item |
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2008
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| _version_ | 1826294665217835008 |
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| author | Morganti, R Manthey, E Crocker, A Oosterloo, T de Zeeuw, P McDermid, R Krajnovic, D Cappellari, M Weijmans, A Sarzi, M |
| author_facet | Morganti, R Manthey, E Crocker, A Oosterloo, T de Zeeuw, P McDermid, R Krajnovic, D Cappellari, M Weijmans, A Sarzi, M |
| author_sort | Morganti, R |
| collection | OXFORD |
| description | A deep H I survey of nearby early-type galaxies carried out with the Westerbork Radio Synthesis telescope has shown that, contrary to expectation, neutral hydrogen is a significant constituent of the ISM in this type of objects located in low density environment. The studied galaxies are part of a representative sample of nearby E and SO for which integral-field spectroscopy using the SAURON spectrograph is available. We present preliminary results on the comparison of the characteristics of the H I with those of the molecular and ionised gas as well as the stellar dynamics and population. |
| first_indexed | 2024-03-07T03:49:11Z |
| format | Conference item |
| id | oxford-uuid:c0a1ae4a-cf1f-4bbf-bb25-c84fa38d10cd |
| institution | University of Oxford |
| last_indexed | 2024-03-07T03:49:11Z |
| publishDate | 2008 |
| record_format | dspace |
| spelling | oxford-uuid:c0a1ae4a-cf1f-4bbf-bb25-c84fa38d10cd2022-03-27T05:55:43ZThe continuing formation of early-type galaxies: an HI surveyConference itemhttp://purl.org/coar/resource_type/c_5794uuid:c0a1ae4a-cf1f-4bbf-bb25-c84fa38d10cdSymplectic Elements at Oxford2008Morganti, RManthey, ECrocker, AOosterloo, Tde Zeeuw, PMcDermid, RKrajnovic, DCappellari, MWeijmans, ASarzi, MA deep H I survey of nearby early-type galaxies carried out with the Westerbork Radio Synthesis telescope has shown that, contrary to expectation, neutral hydrogen is a significant constituent of the ISM in this type of objects located in low density environment. The studied galaxies are part of a representative sample of nearby E and SO for which integral-field spectroscopy using the SAURON spectrograph is available. We present preliminary results on the comparison of the characteristics of the H I with those of the molecular and ionised gas as well as the stellar dynamics and population. |
| spellingShingle | Morganti, R Manthey, E Crocker, A Oosterloo, T de Zeeuw, P McDermid, R Krajnovic, D Cappellari, M Weijmans, A Sarzi, M The continuing formation of early-type galaxies: an HI survey |
| title | The continuing formation of early-type galaxies: an HI survey |
| title_full | The continuing formation of early-type galaxies: an HI survey |
| title_fullStr | The continuing formation of early-type galaxies: an HI survey |
| title_full_unstemmed | The continuing formation of early-type galaxies: an HI survey |
| title_short | The continuing formation of early-type galaxies: an HI survey |
| title_sort | continuing formation of early type galaxies an hi survey |
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