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

M. J. Michalowski, J. M. Castro Ceron, J. L. Wardlow, A. Karska, H. Messias, P. van der Werf, L. K. Hunt, M. Baes, A. J. Castro-Tirado, G. Gentile, J. Hjorth, E. Le Floc'h, R. Perez-Martinez, A. Nicuesa Guelbenzu, J. Rasmussen, J. R. Rizzo, A. Rossi, M. Sanchez-Portal, P. Schady, J. SollermanD. Xu

18 Citations (Scopus)
Original languageEnglish
Article numberA72
JournalAstronomy & Astrophysics
Volume595
ISSN1432-0746
DOIs
Publication statusPublished - 1 Nov 2016

Keywords

  • dust, extinction
  • galaxies: individual: ESO 184-G82
  • galaxies: ISM
  • galaxies: star formation
  • submillimeter: galaxies
  • gamma-ray burst: individual: 980425

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