GRB 980425 host: [C II], [O I], and CO lines reveal recent enhancement of star formation due to atomic gas inflow-Reference-Cited by-同舟云学术

GRB 980425 host: [C II], [O I], and CO lines reveal recent enhancement of star formation due to atomic gas inflow

Published:2016-11 Issue: Volume:595 Page:A72
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Michałowski M. J.,Castro Cerón J. M.,Wardlow J. L.,Karska A.,Messias H.,van der Werf P.,Hunt L. K.,Baes M.,Castro-Tirado A. J.,Gentile G.,Hjorth J.,Le Floc’h E.,Pérez-Martínez R.,Nicuesa Guelbenzu A.,Rasmussen J.,Rizzo J. R.,Rossi A.,Sánchez-Portal M.,Schady P.,Sollerman J.,Xu D.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201629441/pdf

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