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GRB 980425 host: [C II], [O I], and CO lines reveal recent enhancement of star formation due to atomic gas inflow
M. J. Michałowski, J. M. Castro Cerón, 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. Pérez-Martínez, A. Nicuesa Guelbenzu, Jesper Rasmussen, J. R. Rizzo, A. Rossi, M. Sánchez-Portal, P. Schady, J. Sollerman
- University of Edinburgh
- European Space Agency - ESA
- University of Copenhagen
- Nicolaus Copernicus University in Toruń
- University of Lisbon
- Leiden University
- Osservatorio Astrofisico Di Arcetri, Florence
- Universiteit Gent
- Instituto de Astrofísica de Andalucía
- Vrije Universiteit Amsterdam
- European Space Astronomy Centre
- Karl Schwarzschild Observatory
- Centro de Astrobiología
- National Institute for Astrophysics
- Max Planck Institute for Extraterrestrial Physics
- Stockholm University
- Chinese Academy of Sciences
Research output: Contribution to journal › Journal article › Research › peer-review