American Astronomical Society Quick Search:Help  
The Astrophysical Journal
Athens/Institutional login
IOP login: Password:   
Create account | Alerts | Contact us
IOP Publishing | AAS Homepage | ApJ Homepage | This Journal | Search | Authors | Referees | Librarians | User Options | Help |

Modeling the Effects of Dust on Galactic Spectral Energy Distributions from the Ultraviolet to the Millimeter Band

Laura Silva et al 1998 ApJ 509 103-117   doi: 10.1086/306476  Help

   PDF (472 KB) | HTML | References | Articles citing this article

Laura Silva1, Gian Luigi Granato2, Alessandro Bressan2 and Luigi Danese1
1 International School for Advanced Studies, SISSA, Trieste, Italy
2 Osservatorio Astronomico di Padova, Padova, Italy

ABSTRACT. We present models of photometric evolution of galaxies in which the effects of a dusty interstellar medium have been included with particular care. A chemical evolution code follows the star formation rate, the gas fraction, and the metallicity, basic ingredients for the stellar population synthesis. The latter is performed with a grid of integrated spectra of simple stellar populations (SSP) of different ages and metallicities, in which the effects of dusty envelopes around asymptotic giant branch (AGB) stars are included. The residual fraction of gas in the galaxy is divided into two phases: the star-forming molecular clouds and the diffuse medium. The relative amount is a model parameter. The molecular gas is subdivided into clouds of given mass and radius: it is supposed that each SSP is born within the cloud and progressively escapes it. The emitted spectrum of the star-forming molecular clouds is computed with a radiative transfer code. The diffuse dust emission (cirrus) is derived by describing the galaxy as an axially symmetric system, in which the local dust emissivity is consistently calculated as a function of the local field intensity due to the stellar component. Effects of very small grains, subject to temperature fluctuations, as well as polycyclic aromatic hydrocarbons (PAHs) are included. The model is compared and calibrated with available data of normal and starburst galaxies in the local universe, in particular new broadband and spectroscopic Infrared Space Observatory (ISO) observations. It will be a powerful tool to investigate the star formation, the initial mass function (IMF), supernova rate (SNR) in nearby starbursts and normal galaxies, as well as to predict the evolution of luminosity functions of different types of galaxies at wavelengths covering four decades.

Subject headings: dust, extinction; galaxies: ISM; galaxies: spiral; galaxies: starburst; infrared: galaxies; radiative transfer

Print publication: Issue 1 (1998 December 10)
Received 1998 March 16, accepted for publication 1998 July 16

Bookmark and Share Post to CiteUlike | Post to Connotea | Post to Bibsonomy

 

Find related articles





Article options

Authors & Referees

PhysicsWorld, subscribe noweprintweb.org - Your address for E prints
 
Content finder
  Full Search
  Help


  
Setup information is available for Adobe Acrobat.
EndNote, ProCite ® and Reference Manager ® are registered trademarks of ISI Researchsoft.
Copyright © Institute of Physics and IOP Publishing Limited 2009 - electronic design and all rights in the EJs software.
© The American Astronomical Society ("AAS") - the names of any journals published by AAS and the content of all such journals.
Use of this service is subject to compliance with the terms and conditions of use. In particular, reselling and systematic downloading of files is prohibited.
Help: Cookies | Data Protection.