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Titlebook: New Light on Galaxy Evolution; Proceedings of the 1 Ralf Bender,Roger L. Davies Conference proceedings 1996 Springer Science+Business Media

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書(shū)目名稱New Light on Galaxy Evolution
副標(biāo)題Proceedings of the 1
編輯Ralf Bender,Roger L. Davies
視頻videohttp://file.papertrans.cn/666/665432/665432.mp4
叢書(shū)名稱International Astronomical Union Symposia
圖書(shū)封面Titlebook: New Light on Galaxy Evolution; Proceedings of the 1 Ralf Bender,Roger L. Davies Conference proceedings 1996 Springer Science+Business Media
描述The study of the evolution of galaxies has made remarkableprogress in recent years and is currently undergoing a transformationarising from the application of new observational and theoreticaltools. Twenty-one invited reviews, twenty-six contributed papers and137 poster papers cover the wide variety of recent developments,present new insights and demonstrate the rapid increase in ourknowledge about galaxy evolution and formation.
出版日期Conference proceedings 1996
關(guān)鍵詞Dark matter; Galaxy; Universe; stellar
版次1
doihttps://doi.org/10.1007/978-94-009-0229-9
isbn_softcover978-0-7923-3976-2
isbn_ebook978-94-009-0229-9Series ISSN 1743-9213 Series E-ISSN 2352-2186
issn_series 1743-9213
copyrightSpringer Science+Business Media Dordrecht 1996
The information of publication is updating

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The Rate of Supernovae in Normal Galaxieslaxy is known. Constraints to the models are the present chemical content of galaxies but also the present observed SN rate (Arimoto & Yoshi, 1987; Ferrini & Poggianti, 1993; Matteucci, 1994; Renzini ..., 1993; Bressan ..., 1994; Elbaz .., 1995).
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1743-9213 de variety of recent developments,present new insights and demonstrate the rapid increase in ourknowledge about galaxy evolution and formation.978-0-7923-3976-2978-94-009-0229-9Series ISSN 1743-9213 Series E-ISSN 2352-2186
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Disky Ellipticals in the Hubble Sequencehas been suggested that disky ellipticals form together with S0s and spirals a continuous transition in D/B ratio in the Hubble sequence (Bender 1988b, Nieto 1988). However, until the present, this hypothesis had not been investigated throughout.
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Population Synthesis Models formation rate (SFR); and . the rate of chemical enrichment (in some models ...). Most of the recent codes use the isochrone synthesis algorithm, which allows to compute the evolution of a simple stellar population (SSP), and from it, by a convolution integral, the properties of more complex composite stellar populations (CSP).
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Recent Progress in the Search for Black Holes in Galactic Nucleiremarkably well. N-body simulations of an edge-on .(..) model for M32 show that this model is stable. HST spectra should soon provide new and improved constraints on the presence of BHs in quiescent galaxies.
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