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
MartÃn S
(2009)
PHOTODISSOCIATION CHEMISTRY FOOTPRINTS IN THE STARBURST GALAXY NGC 253
in The Astrophysical Journal
Perevoznikov E
(2013)
Short-Wave Charge Instabilities of Weakly Ionized Plasma Flows
in Journal of Engineering Physics and Thermophysics
Troni F
(2013)
Simulation of Current Transport in Polycrystalline CdTe Solar Cells
in Journal of Electronic Materials
Smith K
(2013)
Small-scale structure in the interstellar medium: time-varying interstellar absorption towards ? Velorum
in Monthly Notices of the Royal Astronomical Society
Pilleri P
(2013)
Spatial distribution of small hydrocarbons in the neighborhood of the ultra compact HII region Monoceros R2
in Astronomy & Astrophysics
Vasta M
(2010)
Testing PDR models against ISO fine structure line data for extragalactic sources
in Proceedings of the International Astronomical Union
Vasta M
(2010)
Testing PDR models against ISO fine structure line data for extragalactic sources
in Monthly Notices of the Royal Astronomical Society
Weaver J
(2013)
TH-A-WAB-01: Biomarker Sensing
in Medical Physics
Benedettini M
(2013)
The B1 shock in the L1157 outflow as seen at high spatial resolution?
in Monthly Notices of the Royal Astronomical Society
Codella C
(2010)
The CHESS spectral survey of star forming regions: Peering into the protostellar shock L1157-B1 I. Shock chemical complexity
in Astronomy and 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 |