Chemistry in galaxies at low and high redshifts
Lead Research Organisation:
University College London
Department Name: Physics and Astronomy
Abstract
Abstracts are not currently available in GtR for all funded research. This is normally because the abstract was not required at the time of proposal submission, but may be because it included sensitive information such as personal details.
Organisations
Publications
Bayet E
(2010)
DEUTERATED SPECIES IN EXTRAGALACTIC STAR-FORMING REGIONS
in The Astrophysical Journal
Van Dishoeck E
(2011)
Water in Star-forming Regions with the Herschel Space Observatory (WISH). I. Overview of Key Program and First Results
in Publications of the Astronomical Society of the Pacific
Occhiogrosso A
(2011)
A study of methyl formate in astrochemical environments Methyl formate in astrochemical environments
in Monthly Notices of the Royal Astronomical Society
Collings M. P.
(2011)
LASSIE: Laboratory Astrochemical Surface Science In Europe
in 2010 NASA Laboratory Astrophysics Workshop
Rose S
(2011)
Generating wind time series as a hybrid of measured and simulated data
in Wind Energy
Bayet E
(2011)
CS LINE PROFILES IN HOT CORES
in The Astrophysical Journal
Goldsmith P
(2011)
HERSCHEL MEASUREMENTS OF MOLECULAR OXYGEN IN ORION
in The Astrophysical Journal
Papadopoulos P
(2011)
Extreme cosmic ray dominated regions: a new paradigm for high star formation density events in the Universe Star formation in extreme CRDRs
in Monthly Notices of the Royal Astronomical Society
Christie H
(2011)
Chemistry of dense clumps near moving Herbig-Haro objects Chemistry of dense clumps near HHOs
in Monthly Notices of the Royal Astronomical Society
Tercero B
(2011)
A line-confusion limited millimeter survey of Orion KL II. Silicon-bearing species???
in Astronomy & Astrophysics
Description | We have characterized the dense gas in nearby galaxies |
Exploitation Route | the work will be used to model all submillimeter data of nearby galaxies as well as a pathfinder for new ALMA observations |
Sectors | Other |
Description | We have developed a large suite of astrochemical models that are now routinely used to modl and predict abunadnces of molecules in extragalactic environments |
First Year Of Impact | 2009 |
Sector | Other |