Morphological physical classification galaxies (7 Ergebnisse)
Sprache: Englisch
Verlag: Dordrecht et al., Kluwer,, 1992
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Gr.-8°, original hardcover. 1. ed. XIX, 472 p. Shelfmark on spine, stamp on preliminary page and title, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.
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Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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.
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Zustand: New. Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte, held in Sant Agata Sui Due Golfi, Italy, September 3-7, 1990 The morphological scheme devised by Hubble and followers to classify galaxies has proven over .
Morphological and Physical Classification of Galaxies
. Ed(s): Longo, G.; Capaccioli, M.; Busarello, G. (Osservatorio di Capodimonte, Napoli, Italy)
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Zustand: New. Proceedings of the Fifth International Workshop of the Osservatorio Astronomico di Capodimonte, held in Sant'Agata Sui Due Golfi, Italy, September 3-7, 1990 Editor(s): Longo, G.; Capaccioli, M.; Busarello, G. (Osservatorio di Capodimonte, Napoli, Italy). Series: Astrophysics and Space Science Library. Num Pages: 49…1 pages, biography. BIC Classification: PGM. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 235 x 155 x 26. Weight in Grams: 868. . 1992. Hardback. . . . . Books ship from the US and Ireland.
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Taschenbuch. Zustand: Neu. Neuware - 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 elliptica…ls. 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.
