- Centre National de la Recherche ScientifiqueFR737 papers
- University of CambridgeGB465 papers
- European Southern ObservatoryCL427 papers
- Center for Astrophysics Harvard & SmithsonianUS421 papers
- University of EdinburghGB387 papers
- University of GenevaCH379 papers
- University of WarwickGB331 papers
- Keele UniversityGB330 papers
- Royal ObservatoryGB329 papers
- Instituto de Astrofísica de CanariasES306 papers
- Scottish Universities Physics AllianceGB303 papers
- Space Telescope Science InstituteUS302 papers
55 papers · 1 filter
The Patchy Accretion Disc in HT Cassiopeiae
Sonja Vrielmann, Frederic V. Hessman, Keith Horne
We have reconstructed the temperatures and surface densities in the quiescent accretion disc in HT Cas by performing a "Physical Parameter Eclipse Mapping" analysis of archival UBV…
The 2dF Galaxy Redshift Survey: The amplitudes of fluctuations in the 2dFGRS and the CMB, and implications for galaxy biasing
Ofer Lahav, Sarah L. Bridle, Will J. Percival +26
We compare the amplitudes of fluctuations probed by the 2dF Galaxy Redshift Survey and by the latest measurements of the Cosmic Microwave Background anisotropies. By combining the…
The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe
Licia Verde, Alan F. Heavens, Will J. Percival +27
We compute the bispectrum of the 2dF Galaxy Redshift Survey (2dFGRS) and use it to measure the bias parameter of the galaxies. This parameter quantifies the strength of clustering…
The brown dwarf desert as a consequence of orbital migration
Philip J. Armitage, Ian A. Bonnell
We show that the dearth of brown dwarfs in short-period orbits around Solar-mass stars - the brown dwarf desert - can be understood as a consequence of inward migration within an e…
Profile Shapes for Optically Thick X-ray Emission Lines from Stellar Winds
R. Ignace, K. G. Gayley
We consider the consequences of appreciable line optical depth for the profile shape of X-ray emission lines formed in stellar winds. The hot gas is thought to arise in distributed…
Infrared Signatures of Protoplanetary Disk Evolution
Kenneth Wood, C. J. Lada, J. E. Bjorkman +3
We investigate the observational signatures of a straightforward evolutionary scenario for protoplanetary disks in which the disk mass of small (50 micron) particles decreases homo…