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
Lefloch B
(2010)
The CHESS spectral survey of star forming regions: Peering into the protostellar shock L1157-B1 II. Shock dynamics
in Astronomy and Astrophysics
Busquet G
(2014)
The CHESS survey of the L1157-B1 bow-shock: high and low excitation water vapor
in Astronomy & Astrophysics
Whyatt W
(2010)
The clumpiness of molecular clouds: HCO + (3-2) survey near Herbig-Haro objects
in Astronomy and Astrophysics
Emprechtinger M
(2010)
The distribution of water in the high-mass star-forming region NGC 6334 I
in Astronomy and Astrophysics
Jiménez-Serra I
(2009)
THE EVOLUTION OF MOLECULAR LINE PROFILES INDUCED BY THE PROPAGATION OF C-SHOCK WAVES
in The Astrophysical Journal
Codella C
(2012)
THE HERSCHEL AND IRAM CHESS SPECTRAL SURVEYS OF THE PROTOSTELLAR SHOCK L1157-B1: FOSSIL DEUTERATION
in The Astrophysical Journal
Buckle J
(2010)
The JCMT Legacy Survey of the Gould Belt: a first look at Orion B with HARP
in Monthly Notices of the Royal Astronomical Society
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
Davis C
(2010)
The JCMT Legacy Survey of the Gould Belt: a first look at Taurus with HARP
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 |