Chemistry in galaxies at low and high redshifts
Lead Research Organisation:
University College London
Department Name: Physics and Astronomy
Abstract
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Organisations
Publications
Occhiogrosso A
(2012)
Modelling of c-C 2 H 4 O formation on grain surfaces Modelling of c-C 2 H 4 O formation on grain surfaces
in Monthly Notices of the Royal Astronomical Society
Lerate M
(2010)
Chemical and radiative transfer modelling of the ISO-LWS Fabry-Perot spectra of Orion-KL water lines Modelling far-IR H2O lines from Orion-KL
in Monthly Notices of the Royal Astronomical Society
Occhiogrosso A
(2013)
An improved chemical scheme for the reactions of atomic oxygen and simple unsaturated hydrocarbons - implications for star-forming regions
in Monthly Notices of the Royal Astronomical Society
Rawlings J
(2013)
Episodic explosions in interstellar ices
in Monthly Notices of the Royal Astronomical Society
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
Vasta M
(2010)
Testing PDR models against ISO fine structure line data for extragalactic sources
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
Awad Z
(2014)
Deuterium chemistry of dense gas in the vicinity of low-mass and massive star-forming regions
in Monthly Notices of the Royal Astronomical Society
Bayet E
(2011)
First observations of CN (2-1), HCO+ (3-2) and C2H (3-2) emission lines in the Perseus cluster: constraints on heating mechanisms in the cluster gas Molecules as heating probe in Perseus
in Monthly Notices of the Royal Astronomical Society
Buckle J
(2012)
The JCMT Legacy Survey of the Gould Belt: mapping 13CO and C18O in Orion A GBS HARP survey: Orion A
in Monthly Notices of the Royal Astronomical Society
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 |