H{\alpha} and UV luminosities and star formation rates in a large sample of luminous compact galaxies

TL;DR

This study analyzes star formation rates in about 800 luminous compact galaxies using GALEX UV and Hα data, revealing wide SFR ranges and relationships with galaxy properties, and introduces new starburst evolution metrics.

Contribution

It provides a comprehensive statistical analysis of SFRs in luminous compact galaxies using UV and Hα data, including new parameters for starburst evolution.

Findings

SFRs range from 0.18 to 113 M_sun/yr with median values around 4-5 M_sun/yr.

Regression relations link luminosities to stellar mass, starburst age, and metallicity.

Introduces initial luminosities at zero starburst age as new star formation characteristics.

Abstract

We present the results of a statistical study of the star formation rates (SFR) derived from the Galaxy Evolution Explorer (GALEX) observations in the ultraviolet continuum and in the H\alpha emission line for a sample of about 800 luminous compact galaxies (LCGs). Galaxies in this sample have a compact structure and include one or several regions of active star formation. Global galaxy characteristics (metallicity, luminosity, stellar mass) are intermediate between ones of the nearby blue compact dwarf (BCD) galaxies and Lyman-break galaxies (LBGs) at high redshifts z > 2 - 3. SFRs were corrected for interstellar extinction which was derived from the optical Sloan Digital Sky Survey (SDSS) spectra. We find that SFRs derived from the galaxy luminosities in the far ultraviolet (FUV) and near ultraviolet (NUV) ranges vary in a wide range from 0.18 M_Sun/yr to 113 M_Sun/yr with median values of 3.8 M_Sun/yr and 5.2 M_Sun/yr, respectively. Simple regression relations are found for luminosities L(H\alpha) and L(UV) as functions of the mass of the young stellar population, the starburst age, and the galaxy metallicity. We consider the evolution of L(H\alpha), L(FUV) and L(NUV) with a starburst age and introduce new characteristics of star formation, namely the initial H\alpha, FUV and NUV luminosities at zero starburst age.