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
Jiménez-Serra I
(2014)
DETECTABILITY OF GLYCINE IN SOLAR-TYPE SYSTEM PRECURSORS
in The Astrophysical Journal
Kama M
(2010)
The methanol lines and hot core of OMC2-FIR4, an intermediate-mass protostar, with Herschel /HIFI
in Astronomy and Astrophysics
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
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
Liao J
(2014)
Yb3+ concentration dependence of upconversion luminescence in Y2Sn2O7:Yb3+/Er3+ nanophosphors
in Journal of Materials Science
Lis D
(2010)
Herschel /HIFI discovery of interstellar chloronium (H 2 Cl + )
in Astronomy and Astrophysics
Liseau R
(2012)
Multi-line detection of O 2 toward ? Ophiuchi A
in Astronomy & Astrophysics
López A
(2014)
Laboratory characterization and astrophysical detection of vibrationally excited states of vinyl cyanide in Orion-KL
in Astronomy & Astrophysics
Makrymallis A
(2014)
UNDERSTANDING THE FORMATION AND EVOLUTION OF INTERSTELLAR ICES: A BAYESIAN APPROACH
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 |