Morphological and Physical Classification of Galaxies: Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte Held in Sant’Agata Sui Due Golfi, Italy, September 3–7, 1990
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1992
|
| Schriftenreihe: | Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews
178 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | The morphological scheme devised by Hubble and followers to classify galaxies has proven over many decades to be quite effective in directing our quest for the fundamental pa rameters describing the extragalactic manifold. This statement is however far more true for spirals than for ellipticals. Echoing the concluding remarks in Scott Tremaine's sum mary talk at the Princeton meeting on Structure and Dynamics of Elliptical Galaxies, "the Hubble classification of spirals is useful because many properties of spirals (gas con tent, spiral arm morphology, bulge prominence, etc. ) all correlate with Hubble time. By contrast, almost nothing correlates with the elliptical Hubble sequence El to E7. " During the last few years much effort has been put into the search for a more meaningful classification of ellipticals than Hubble's. Concomitantly, forwarded by some provocative conjectures by R. Michard, the classical question of whether E galaxies form a physically homogeneous family has been brushed up once more. Results of these and other parallel studies look rather promising and point to suture part of the dichotomy between ellipticals and disk galaxies which had become popular in the early eighties, owing to dynamical arguments. At the same time it appears more and more clear that, besides the usual genetic varieties of galaxies, products of environmental evolution must also be contemplated in building our modern picture of the "reign of galaxies" . The above considerations prompted us to solicit Prof |
| Beschreibung: | 1 Online-Ressource (XIX, 472 p) |
| ISBN: | 9789401125222 9789401051132 |
| ISSN: | 0067-0057 |
| DOI: | 10.1007/978-94-011-2522-2 |
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| 245 | 1 | 0 | |a Morphological and Physical Classification of Galaxies |b Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte Held in Sant’Agata Sui Due Golfi, Italy, September 3–7, 1990 |c edited by G. Longo, M. Capaccioli, G. Busarello |
| 246 | 1 | 3 | |a Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte, held in Sant'Agata Sui Due Golfi, Italy, September 3-7, 1990 |
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| 490 | 0 | |a Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews |v 178 |x 0067-0057 | |
| 500 | |a The morphological scheme devised by Hubble and followers to classify galaxies has proven over many decades to be quite effective in directing our quest for the fundamental pa rameters describing the extragalactic manifold. This statement is however far more true for spirals than for ellipticals. Echoing the concluding remarks in Scott Tremaine's sum mary talk at the Princeton meeting on Structure and Dynamics of Elliptical Galaxies, "the Hubble classification of spirals is useful because many properties of spirals (gas con tent, spiral arm morphology, bulge prominence, etc. ) all correlate with Hubble time. By contrast, almost nothing correlates with the elliptical Hubble sequence El to E7. " During the last few years much effort has been put into the search for a more meaningful classification of ellipticals than Hubble's. Concomitantly, forwarded by some provocative conjectures by R. Michard, the classical question of whether E galaxies form a physically homogeneous family has been brushed up once more. Results of these and other parallel studies look rather promising and point to suture part of the dichotomy between ellipticals and disk galaxies which had become popular in the early eighties, owing to dynamical arguments. At the same time it appears more and more clear that, besides the usual genetic varieties of galaxies, products of environmental evolution must also be contemplated in building our modern picture of the "reign of galaxies" . The above considerations prompted us to solicit Prof | ||
| 650 | 4 | |a Physics | |
| 650 | 4 | |a Astronomy, Observations and Techniques | |
| 700 | 1 | |a Capaccioli, M. |e Sonstige |4 oth | |
| 700 | 1 | |a Busarello, G. |e Sonstige |4 oth | |
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Datensatz im Suchindex
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| dewey-full | 520 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 520 - Astronomy and allied sciences |
| dewey-raw | 520 |
| dewey-search | 520 |
| dewey-sort | 3520 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-011-2522-2 |
| format | Electronic eBook |
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| id | DE-604.BV042415876 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:58Z |
| institution | BVB |
| isbn | 9789401125222 9789401051132 |
| issn | 0067-0057 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027851369 |
| oclc_num | 863785844 |
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| physical | 1 Online-Ressource (XIX, 472 p) |
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| publishDate | 1992 |
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| series2 | Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews |
| spelling | Longo, G. Verfasser aut Morphological and Physical Classification of Galaxies Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte Held in Sant’Agata Sui Due Golfi, Italy, September 3–7, 1990 edited by G. Longo, M. Capaccioli, G. Busarello Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte, held in Sant'Agata Sui Due Golfi, Italy, September 3-7, 1990 Dordrecht Springer Netherlands 1992 1 Online-Ressource (XIX, 472 p) txt rdacontent c rdamedia cr rdacarrier Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews 178 0067-0057 The morphological scheme devised by Hubble and followers to classify galaxies has proven over many decades to be quite effective in directing our quest for the fundamental pa rameters describing the extragalactic manifold. This statement is however far more true for spirals than for ellipticals. Echoing the concluding remarks in Scott Tremaine's sum mary talk at the Princeton meeting on Structure and Dynamics of Elliptical Galaxies, "the Hubble classification of spirals is useful because many properties of spirals (gas con tent, spiral arm morphology, bulge prominence, etc. ) all correlate with Hubble time. By contrast, almost nothing correlates with the elliptical Hubble sequence El to E7. " During the last few years much effort has been put into the search for a more meaningful classification of ellipticals than Hubble's. Concomitantly, forwarded by some provocative conjectures by R. Michard, the classical question of whether E galaxies form a physically homogeneous family has been brushed up once more. Results of these and other parallel studies look rather promising and point to suture part of the dichotomy between ellipticals and disk galaxies which had become popular in the early eighties, owing to dynamical arguments. At the same time it appears more and more clear that, besides the usual genetic varieties of galaxies, products of environmental evolution must also be contemplated in building our modern picture of the "reign of galaxies" . The above considerations prompted us to solicit Prof Physics Astronomy, Observations and Techniques Capaccioli, M. Sonstige oth Busarello, G. Sonstige oth https://doi.org/10.1007/978-94-011-2522-2 Verlag Volltext |
| spellingShingle | Longo, G. Morphological and Physical Classification of Galaxies Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte Held in Sant’Agata Sui Due Golfi, Italy, September 3–7, 1990 Physics Astronomy, Observations and Techniques |
| title | Morphological and Physical Classification of Galaxies Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte Held in Sant’Agata Sui Due Golfi, Italy, September 3–7, 1990 |
| title_alt | Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte, held in Sant'Agata Sui Due Golfi, Italy, September 3-7, 1990 |
| title_auth | Morphological and Physical Classification of Galaxies Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte Held in Sant’Agata Sui Due Golfi, Italy, September 3–7, 1990 |
| title_exact_search | Morphological and Physical Classification of Galaxies Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte Held in Sant’Agata Sui Due Golfi, Italy, September 3–7, 1990 |
| title_full | Morphological and Physical Classification of Galaxies Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte Held in Sant’Agata Sui Due Golfi, Italy, September 3–7, 1990 edited by G. Longo, M. Capaccioli, G. Busarello |
| title_fullStr | Morphological and Physical Classification of Galaxies Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte Held in Sant’Agata Sui Due Golfi, Italy, September 3–7, 1990 edited by G. Longo, M. Capaccioli, G. Busarello |
| title_full_unstemmed | Morphological and Physical Classification of Galaxies Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte Held in Sant’Agata Sui Due Golfi, Italy, September 3–7, 1990 edited by G. Longo, M. Capaccioli, G. Busarello |
| title_short | Morphological and Physical Classification of Galaxies |
| title_sort | morphological and physical classification of galaxies proceedings of the fifth international workshop of the osservatorio astronomico di capodimonte held in sant agata sui due golfi italy september 3 7 1990 |
| title_sub | Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte Held in Sant’Agata Sui Due Golfi, Italy, September 3–7, 1990 |
| topic | Physics Astronomy, Observations and Techniques |
| topic_facet | Physics Astronomy, Observations and Techniques |
| url | https://doi.org/10.1007/978-94-011-2522-2 |
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