SIMBAD references

2020MNRAS.499L.105M - Mon. Not. R. Astron. Soc., 499, L105-L110 (2020/November-3)

The discovery of the most UV-Ly α luminous star-forming galaxy: a young, dust- and metal-poor starburst with QSO-like luminosities.

MARQUES-CHAVES R., ALVAREZ-MARQUEZ J., COLINA L., PEREZ-FOURNON I., SCHAERER D., DALLA VECCHIA C., HASHIMOTO T., JIMENEZ-ANGEL C. and SHU Y.

Abstract (from CDS):

We report the discovery of BOSS-EUVLG1 at z = 2.469, by far the most luminous, almost un-obscured star-forming galaxy known at any redshift. First classified as a QSO within the Baryon Oscillation Spectroscopic Survey, follow-up observations with the Gran Telescopio Canarias reveal that its large luminosity, MUV ≃ -24.40 and log(LLyα/erg s–1) ≃ 44.0, is due to an intense burst of star formation, and not to an active galactic nucleus or gravitational lensing. BOSS-EUVLG1 is a compact (reff ≃ 1.2 kpc), young (4-5 Myr) starburst with a stellar mass log(M*/M☉) = 10.0 ± 0.1 and a prodigious star formation rate of ≃1000 M☉ yr–1. However, it is metal- and dust-poor [12 + log(O/H) = 8.13 ± 0.19, E(B - V) ≃ 0.07, log(LIR/LUV) < -1.2], indicating that we are witnessing the very early phase of an intense starburst that has had no time to enrich the ISM. BOSS-EUVLG1 might represent a short-lived (<100 Myr), yet important phase of star-forming galaxies at high redshift that has been missed in previous surveys. Within a galaxy evolutionary scheme, BOSS-EUVLG1 could likely represent the very initial phases in the evolution of massive quiescent galaxies, even before the dusty star-forming phase.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): galaxies: formation - galaxies: high-redshift

Simbad objects: 1

goto Full paper

goto View the references in ADS

To bookmark this query, right click on this link: simbad:2020MNRAS.499L.105M and select 'bookmark this link' or equivalent in the popup menu