Visiting Fellowships, IoA, 2010 - 2013
Lead Research Organisation:
University of Cambridge
Department Name: Institute of Astronomy
Abstract
The rolling STFC Visitor Programme at the Institute of Astronomy benefits all the research undertaken at the Institute by attracting leading astronomers from around the world to Cambridge to share ideas and develop long-term collaborations. For many years the Institute has maintained a strong visitor programme with a healthy reputation and this creates a significant 'mulitplier effect' by which yet more distinguished visitors are attracted to visit on their own funding. The Institute is a key partner in many national and international projects, all of which will both attract active visiting scientists and benefit from the overall visitor programme.
Organisations
People |
ORCID iD |
Robert C Kennicutt (Principal Investigator) |
Publications
Dobbs C
(2011)
Why are most molecular clouds not gravitationally bound? Unbound molecular clouds
in Monthly Notices of the Royal Astronomical Society
Deason A
(2011)
Mismatch and misalignment: dark haloes and satellites of disc galaxies Mismatch and misalignment
in Monthly Notices of the Royal Astronomical Society
De Marco B
(2011)
PG 1211+143: probing high-frequency lags in a high-mass active galactic nucleus PG 1211+143
in Monthly Notices of the Royal Astronomical Society: Letters
Crain R
(2010)
X-ray coronae in simulations of disc galaxy formation X-ray coronae of disc galaxies
in Monthly Notices of the Royal Astronomical Society
Conn A
(2011)
A BAYESIAN APPROACH TO LOCATING THE RED GIANT BRANCH TIP MAGNITUDE. I.
in The Astrophysical Journal
Collins M
(2011)
The scatter about the 'Universal' dwarf spheroidal mass profile: a kinematic study of the M31 satellites And V and And VI Scatter about Universal dwarf spheroidal mass
in Monthly Notices of the Royal Astronomical Society
Clarke C
(2013)
Evolutionary constraints on the planetary hypothesis for transition discs
in Monthly Notices of the Royal Astronomical Society: Letters
Carswell R
(2012)
The kinetic temperature in a damped Lyman a absorption system in Q2206-199 - an example of the warm neutral medium Warm neutral gas towards Q2206-199
in Monthly Notices of the Royal Astronomical Society
Calverley A
(2011)
Measurements of the ultraviolet background at 4.6 < z < 6.4 using the quasar proximity effect? Proximity-effect measurements of the UVB at high redshift
in Monthly Notices of the Royal Astronomical Society