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arXiv.org e-Print Archive
Preprint . 2000
Data sources: arXiv.org e-Print Archive
https://dx.doi.org/10.48550/ar...
Article . 2000
License: arXiv Non-Exclusive Distribution
Data sources: Datacite
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Bulges

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Jan 2000Embargo end date: 01 Jan 2000Publisher:arXiv
Authors: Molla, M.; Ferrini, F.; Gozzi, G.;

doi: 10.48550/arxiv.astro-ph/0003006

arXiv: astro-ph/0003006

Abstract

We model the evolution of the galactic bulge and of the bulges of a selected sample of external spiral galaxies, via the multiphase multizone evolution model. We address a few questions concerning the role of the bulges within galactic evolution schemes and the properties of bulge stellar populations. We provide solutions to the problems of chemical abundances and spectral indices, the two main observational constraints to bulge structure.

15 pages, 10 figures, to be published in MNRAS

Related Organizations
Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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    influence
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selected citations
These citations are derived from selected sources.
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
Average
Average
Average
Green
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