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
Offner S
(2013)
MODELING THE ATOMIC-TO-MOLECULAR TRANSITION AND CHEMICAL DISTRIBUTIONS OF TURBULENT STAR-FORMING CLOUDS
in The Astrophysical Journal
Offner S
(2014)
An alternative accurate tracer of molecular clouds: the 'XCi-factor'
in Monthly Notices of the Royal Astronomical Society: Letters
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
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
Perevoznikov E
(2013)
Short-Wave Charge Instabilities of Weakly Ionized Plasma Flows
in Journal of Engineering Physics and Thermophysics
Pilleri P
(2013)
Spatial distribution of small hydrocarbons in the neighborhood of the ultra compact HII region Monoceros R2
in Astronomy & Astrophysics
Prins C
(2013)
An inverse method for the design of TIR collimators to achieve a uniform color light beam
in Journal of Engineering Mathematics
RANI S
(2013)
Two-dimensional deformation of a uniform half-space due to non-uniform movement accompanying a long vertical tensile fracture
in Journal of Earth System Science
Rawlings J
(2013)
Episodic explosions in interstellar ices
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 |