Star Formation Rate at z = 0.2 derived from H_alpha luminosities: constraint on the reddening

Laurence Tresse; Steve J. Maddox

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arXiv · astro-ph/9712130

Star Formation Rate at z = 0.2 derived from H_alpha luminosities: constraint on the reddening

Laurence Tresse·Steve J. Maddox

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Abstract

We discuss the relative merits of using UV and H_alpha as star formation indicators from galaxy surveys. In particular, comparing UV and H_alpha in the CFRS gives a limit of a factor 2.5 for the UV(2800 Angs.) flux extinction from dust, using the conversion factors of Madau et al. 1998 (Salpeter IMF, 0.1-125 solar mass). Our strong correlation between B and H_alpha luminosities argues for a universal IMF slope. The H_alpha luminosity function at z = 0.2 shows a faint end slope of alpha = -1.35, which is consistent with fading of short bursts of star formation. We also discuss the contribution of AGN to UV and H_alpha luminosities.

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Laurence Tresse, Steve J. Maddox. 1997-12-09. Star Formation Rate at z = 0.2 derived from H_alpha luminosities: constraint on the reddening. https://arxiv.org/abs/astro-ph/9712130

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