The importance of following the evolution of the dust in galaxies on their SEDs

被引：0
|
作者：
Schurer, A. [1 ,2 ]
Calura, F. [3 ]
Silva, L. [3 ]
Pipino, A. [4 ]
Granato, G. L. [3 ]
Matteucci, F. [3 ,5 ]
Maiolino, R. [6 ]
机构：
[1] SISSA ISAS, Via Beirut 2-4, I-34014 Trieste, Italy
[2] Osserv Astron Padova, INAF, I-35122 Padua, Italy
[3] Osserv Astron Trieste, INAF, I-34131 Trieste, Italy
[4] Univ Oxford, Astrophys, Oxford OX1 3RH, England
[5] Univ Trieste, Dipartimento Astron, INAF, I-34131 Trieste, Italy
[6] Osserv Astron Roma, INAF, Monte Porzio Catone, Italy
来源：
LOW-METALLICITY STAR FORMATION: FROM THE FIRST STARS TO DWARF GALAXIES | 2008年 / 255期
关键词：
ISM: abundances; ISM: dust; extinction; galaxies: abundances; galaxies: evolution;
D O I：
10.1017/S1743921308024721
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present photometric evolution of galaxies ill which, in addition to the stellar component, the effects of all evolving dusty interstellar have been included with particular care. Starting from the work of Calura, Pipino & Matteucci (2008)7 in which chemical evolution models have been used to study the evolution of both the, gas and dust, component's of die interstellar medium in spiral, elliptical and irregular galaxies, it has been possible to combine these models with a spectrophotometric stellar synthesis code that includes dust reprocessing (GRASIL) (Silva 1998) to analyse the evolution of the Spectral Energy Distributions (SED) of these galaxies. We test our models against observed SEDs both in the local universe and at high redshift. The, importance of following the dust evolution is investigated by comparing our results with Chose obtained by adopting simple assumptions to treat this component. Possible errors front assuming a Milky, Way (lust composition and a dust-to-gas ratio scaling with the metallicity particularly in young galaxies, ellipticals and low metallicity galaxies dire highlighted.
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收藏
页码：147 / +
页数：2
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