The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types-Reference-Cited by-同舟云学术

The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types

Published:2014-08 Issue: Volume:568 Page:A62
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

De Looze Ilse,Cormier Diane,Lebouteiller Vianney,Madden Suzanne,Baes Maarten,Bendo George J.,Boquien Médéric,Boselli Alessandro,Clements David L.,Cortese Luca,Cooray Asantha,Galametz Maud,Galliano Frédéric,Graciá-Carpio Javier,Isaak Kate,Karczewski Oskar Ł.,Parkin Tara J.,Pellegrini Eric W.,Rémy-Ruyer Aurélie,Spinoglio Luigi,Smith Matthew W. L.,Sturm Eckhard

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201322489/pdf

Reference174 articles.

1. DUST-BOUNDED ULTRALUMINOUS INFRARED GALAXIES: MODEL PREDICTIONS FOR INFRARED SPECTROSCOPIC SURVEYS

2. Excitation Rate Coefficients for Fine‐Structure Transitions in O iii

3. Near‐Infrared and Star‐forming Properties of Local Luminous Infrared Galaxies

4. Common-Resolution Convolution Kernels for Space- and Ground-Based Telescopes

5. YOUNG STELLAR POPULATIONS AND STAR CLUSTERS IN NGC 1705

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