We use the self-consistent model technique developed by Martín-Manjón et
al. (2008) that combines the chemical evolution with stellar population
synthesis and photo-ionization codes, to study the star formation scenarios
capable of reproducing the observed properties of star-forming galaxies.
The comparison of our model results with a database of HII galaxies shows
that the observed spectra and colors of the present burst and the older
underlying population are reproduced by models in a bursting scenario with star
formation efficiency involving close to 20 per cent of the total mass of gas,
and inter-burst times longer than 100 Myr, and more probably around 1 Gyr.
Other modes like gasping and continuous star formation are not favored.
Описание
[1111.1925] Evolution of star forming dwarf galaxies: Characterizing the star formation scenarios
%0 Generic
%1 Martín-Manjón2011
%A Martín-Manjón, M. L.
%A Mollá, M.
%A Díaz, A. I.
%A Terlevich, R.
%D 2011
%K dwarf formation galaxies star
%T Evolution of star forming dwarf galaxies: Characterizing the star
formation scenarios
%U http://arxiv.org/abs/1111.1925
%X We use the self-consistent model technique developed by Martín-Manjón et
al. (2008) that combines the chemical evolution with stellar population
synthesis and photo-ionization codes, to study the star formation scenarios
capable of reproducing the observed properties of star-forming galaxies.
The comparison of our model results with a database of HII galaxies shows
that the observed spectra and colors of the present burst and the older
underlying population are reproduced by models in a bursting scenario with star
formation efficiency involving close to 20 per cent of the total mass of gas,
and inter-burst times longer than 100 Myr, and more probably around 1 Gyr.
Other modes like gasping and continuous star formation are not favored.
@misc{Martín-Manjón2011,
abstract = { We use the self-consistent model technique developed by Mart\'in-Manj\'on et
al. (2008) that combines the chemical evolution with stellar population
synthesis and photo-ionization codes, to study the star formation scenarios
capable of reproducing the observed properties of star-forming galaxies.
The comparison of our model results with a database of HII galaxies shows
that the observed spectra and colors of the present burst and the older
underlying population are reproduced by models in a bursting scenario with star
formation efficiency involving close to 20 per cent of the total mass of gas,
and inter-burst times longer than 100 Myr, and more probably around 1 Gyr.
Other modes like gasping and continuous star formation are not favored.
},
added-at = {2011-11-09T22:22:51.000+0100},
author = {Martín-Manjón, M. L. and Mollá, M. and Díaz, A. I. and Terlevich, R.},
biburl = {https://www.bibsonomy.org/bibtex/269c71883154b056951df37ebe9642f7e/miki},
description = {[1111.1925] Evolution of star forming dwarf galaxies: Characterizing the star formation scenarios},
interhash = {8b1f2b2ba665a965aee84489a7194481},
intrahash = {69c71883154b056951df37ebe9642f7e},
keywords = {dwarf formation galaxies star},
note = {cite arxiv:1111.1925
Comment: 18 pages, 10 figures, to be published in MNRAS},
timestamp = {2011-11-09T22:22:51.000+0100},
title = {Evolution of star forming dwarf galaxies: Characterizing the star
formation scenarios},
url = {http://arxiv.org/abs/1111.1925},
year = 2011
}