Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Galaxy Astrophysics
Scientist
Onsala Space Observatory, Sweden
Chalmers Univ
Chalmers University of Technology, Sweden
MPIFR
Steward Observatory, Tucson, AZ
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA
Minnesota, University, Minneapolis, Minn.
Onsala Space Observatory, Sweden; Steward Observatory, Tucson, AZ
Chalmers Technical University, Goteborg, Sweden; Leiden
Onsala Space Observatory, Chalmers University of Technology, 43992 Onsala, Sweden Space Observatory, Dept. of Earth and Space Sciences, Chalmers University of Technology, 43992, Onsala, Sweden
University of Arizona, Tucson, AZ
Chalmers Centre for Astrophysics and Space Science, Onsala Space Observatory, Chalmers University of Technology, 43 992 Onsala, Sweden Space Observatory, Department of Earth and Space Sciences, Chalmers University of Technology, 439 92, Onsala, Sweden
Onsala Space Observatory
Onsala Space Observatory, Onsala Space Observatory, 439 92, Onsala, Sweden
Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass.
Onsala Space Observatory, 439 92 Onsala, Sweden Observatory, University of Arizona
Centre for Astrophysics and Space Science, Chalmers University of Technology, Onsala Space Observatory, 43992 Onsala, Sweden Sterrewacht, Netherlands; Steward Observatory, Tucson, AZ
Onsala Space Observatory, S-43992 Onsala, Sweden
Smithsonian Astrophysical Observatory and Harvard College Observatory, Cambridge, Mass.
Onsala Space Observatory, Chalmers University of Technology, 439 92 Onsala, Sweden
Onsala Space Observatory, Chalmers University of Technology, SE-43992 Onsala, Sweden
Leiden, Sterrewacht, Netherlands; Onsala Space Observatory, Sweden; Steward Observatory, Tucson, AZ
Onsala Space Obs.
Arizona Univ., Tucson, AZ
L
10 to the 12th solar luminosity starbursts and shocked molecular hydrogen in the colliding galaxies ARP 220 (= IC 4553) and NGC 6240
12C18^O(3-2) map of rho Oph A (Liseau+,
7mm spectral survey of PKS 1830-211 (Muller+, 2011)
A 5 GHz survey of infrared sources
A chemical inventory of the S-type AGB star χ Cygni based on Herschel/HIFI observations of circumstellar line emission. The importance of non-LTE chemical processes in a dynamical region
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Profile ID: LFWR-SCP-P-70450