HERSCHEL HIFI OBSERVATIONS OF O-2 TOWARD ORION: SPECIAL CONDITIONS FOR SHOCK ENHANCED EMISSION
Artikel i vetenskaplig tidskrift, 2014
line survey
wave-astronomy-satellite
interstellar molecular clouds
aperture synthesis
massive stars
cologne database
hot core
star-formation
rho-ophiuchi
temporal evolution
Författare
Jo-Hsin Chen
Jet Propulsion Laboratory, California Institute of Technology
Paul F. Goldsmith
Jet Propulsion Laboratory, California Institute of Technology
Serena Viti
University College London (UCL)
Ronald Snell
University of Massachusetts
D. Lis
Université Pierre et Marie Curie (UPMC)
California Institute of Technology (Caltech)
A.O. Benz
Eidgenössische Technische Hochschule Zürich (ETH)
E. A. Bergin
University of Michigan
John H Black
Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik
P. Caselli
Max-Planck-Gesellschaft
P. J. Encrenaz
Centre national de la recherche scientifique (CNRS)
E. Falgarone
Centre national de la recherche scientifique (CNRS)
Javier R. Goicoechea
Consejo Superior de Investigaciones Científicas (CSIC)
Åke Hjalmarson
Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik
David Hollenbach
SETI Institute
Michael J. Kaufman
San Jose State University
G. J. Melnick
Harvard-Smithsonian Center for Astrophysics
D. A. Neufeld
Johns Hopkins University
Laurent Pagani
LERMA - Laboratoire d'Etudes du Rayonnement et de la Matiere en Astrophysique et Atmospheres
F. F. S. van der Tak
Netherlands Institute for Space Research (SRON)
Rijksuniversiteit Groningen
E. F. van Dishoeck
Universiteit Leiden
Max-Planck-Gesellschaft
U. A. Yildiz
Jet Propulsion Laboratory, California Institute of Technology
Astrophysical Journal
0004-637X (ISSN) 1538-4357 (eISSN)
Vol. 793 2 Article nr. 111 - 111Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
DOI
10.1088/0004-637X/793/2/111