WISE Discovery of Low Metallicity Blue Compact Dwarf Galaxies

TL;DR

This paper reports the discovery of two new low metallicity blue compact dwarf galaxies using WISE infrared data, providing insights into star formation in extreme environments and proposing a new identification method.

Contribution

The study introduces a novel approach to identify low metallicity BCDs via mid-infrared colors and presents the discovery of two such galaxies with detailed spectroscopic analysis.

Findings

Both galaxies have metallicities below 1/10 Zsun.

They exhibit young star-forming regions less than 5 Myr old.

Star formation rates are 2.6 and 10.9 Msun/yr respectively.

Abstract

We report two new low metallicity blue compact dwarf galaxies (BCDs), WISEP J080103.93+264053.9 (hereafter W0801+26) and WISEP J170233.53+180306.4 (hereafter W1702+18), discovered using the Wide-field Infrared Survey Explorer (WISE). We identified these two BCDs from their extremely red colors at mid-infrared wavelengths, and obtained follow-up optical spectroscopy using the Low Resolution Imaging Spectrometer on Keck I. The mid-infrared properties of these two sources are similar to the well studied, extremely low metallicity galaxy SBS 0335-052E. We determine metallicities of 12 + log(O/H) = 7.75 and 7.63 for W0801+26 and W1702+18, respectively, placing them amongst a very small group of very metal deficient galaxies (Z < 1/10 Zsun). Their > 300 Angstrom Hbeta equivalent widths, similar to SBS 0335-052E, imply the existence of young (< 5 Myr) star forming regions. We measure star formation rates of 2.6 and 10.9 Msun/yr for W0801+26 and W1702+18, respectively. These BCDs, showing recent star formation activity in extremely low metallicity environments, provide new laboratories for studying star formation in extreme conditions and are low-redshift analogs of the first generation of galaxies to form in the universe. Using the all-sky WISE survey, we discuss a new method to identify similar star forming, low metallicity BCDs.