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
Kama M
(2010)
The methanol lines and hot core of OMC2-FIR4, an intermediate-mass protostar, with Herschel /HIFI
in Astronomy and Astrophysics
Graves S
(2010)
The JCMT Legacy Survey of the Gould Belt: a first look at Serpens with HARP GBS: first look at Serpens
in Monthly Notices of the Royal Astronomical Society
Molinari S
(2010)
Hi-GAL: The Herschel Infrared Galactic Plane Survey
in Publications of the Astronomical Society of the Pacific
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
Bacmann A
(2010)
First detection of ND in the solar-mass protostar IRAS16293-2422
in Astronomy and Astrophysics
Bayet E
(2010)
Molecular tracers of filamentary CO emission regions surrounding the central galaxies of clusters
in Astronomy and Astrophysics
Ossenkopf V
(2010)
Detection of interstellar oxidaniumyl: Abundant H 2 O + towards the star-forming regions DR21, Sgr B2, and NGC6334
in Astronomy and Astrophysics
Vastel C
(2010)
Ortho-to-para ratio of interstellar heavy water
in Astronomy and Astrophysics
Busquet G
(2010)
The NH 2 D/NH 3 ratio toward pre-protostellar cores around the UC$\ion{H}{ii}$ region in IRAS 20293+3952
in Astronomy and Astrophysics
Islam F
(2010)
FORMATION PUMPING OF MOLECULAR HYDROGEN IN DARK CLOUDS
in The Astrophysical Journal
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 |