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

Research output: Contribution to journalJournal articlepeer-review

  • 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
  • E. Le Floc'h
  • R. Perez-Martinez
  • A. Nicuesa Guelbenzu
  • J. Rasmussen
  • J. R. Rizzo
  • A. Rossi
  • M. Sanchez-Portal
  • P. Schady
  • J. Sollerman
  • D. Xu
Original languageEnglish
Article numberA72
JournalAstronomy & Astrophysics
Volume595
ISSN1432-0746
DOIs
Publication statusPublished - 4 Nov 2016

    Research areas

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

ID: 173093253