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arXiv.org e-Print Archive
Preprint . 2003
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Article . 2003
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Article . 2003
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Article . 2003
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Astrophysics and Space Science
Article . 2003 . Peer-reviewed
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Article . 2003
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Galactic Evolution along the Hubble Sequence

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Preprint , Other literature type 01 Jan 2003Embargo end date: 01 Jan 2003 English Publisher:Springer NetherlandsJournal:Astrophysics and Space Science, volume 284, pages 767-770 (issn: 0004-640X, eissn: 1572-946X, Copyright policy )
Authors: Mollá, Mercedes; Díaz Beltrán, Ángeles Isabel;

doi: 10.1007/978-94-017-3315-1_93 , 10.1023/a:1024056802504 , 10.48550/arxiv.astro-ph/0302081

arXiv: http://arxiv.org/abs/astro-ph/0302081

handle: 10486/13807

Galactic Evolution along the Hubble Sequence

Abstract

A generalization of the multiphase chemical evolution model applied to a wide set of theoretical galaxies is shown. This set of models has been computed by using the so-called Universal Rotation Curve from Persic, Salucci & Steel to calculate the radial mass distributions of each theoretical galaxy. By assuming that the molecular cloud and star formation efficiencies depend on the morphological type of each galaxy, we construct a bi-parametric grid of models whose results are valid in principle for any spiral galaxy, of given maximum rotation velocity or total mass, and morphological type.

Proceedings of the Euroconference "The Evolution of Galaxies. III..." (Kiel 2002)

Related Organizations
Keywords

Galaxies: abundances, Astrophysics (astro-ph), spirals [Galaxies], abundances [Galaxies], Física, Galaxies: evolution, FOS: Physical sciences, evolution [Galaxies], Astrophysics, Galaxies: spirals

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
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Average
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