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

Author(s):: Michalowski, M.; Castro Cerón, J.; Wardlow, J.; Karska, A.; Messias, H.; Werf, P.P. van der (0000-0002-4389-832x); Hunt, L.; Baes, M.; Castro-Tirado, A.; Gentile, G.; Hjorth, J.; Le Floch, E.; Pérez-Martínez, R.; Nicuesa Guelbenzu, A.; Rasmussen, J.; Rizzo, J.; Rossi, A.; Sánchez-Portal, M.; Schady, P.; Sollerman, J.; Xu, D.

Published: 2016
Publication type: Article / Letter to editor

Date issued: 2016
Language: English
Is part of: Astronomy & Astrophysics (2016), Vol. 595, p. A72
hdl: 1887/47197
doi: 10.1051/0004-6361/201629441
URL: http://adsabs.harvard.edu/abs/2016A%26A...595A..72M