Star formation rate in Holmberg IX dwarf galaxy

Star formation rate in Holmberg IX dwarf galaxy

In this paper we use previously determined Hα fluxes for dwarf galaxy Holmberg IX (Arbutina et al. 2009) to calculate star formation rate (SFR) in this galaxy. We discuss possible contaminations of Hα flux and, for the first time, we take into account optical emission from supernova remnant...

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Bibliographic Details
Main Author:	Anđelić M.M.
Format:	Article
Language:	English
Published:	Astronomical Observatory, Department of Astronomy, Belgrade 2011-01-01
Series:	Serbian Astronomical Journal
Subjects:	galaxies: dwarf galaxies: ISM HII regions ISM: supernova remnants stars: formation
Online Access:	http://www.doiserbia.nb.rs/img/doi/1450-698X/2011/1450-698X1183071A.pdf

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