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

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

E-ISSN: 1432-0746|595|issue|A72-A72

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.595, Iss.issue, 2016-11, pp. : A72-A72

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract