| dc.contributor.author | Hartley, L.E. | |
| dc.contributor.author | Drew, J.E. | |
| dc.contributor.author | Long, K.S. | |
| dc.date.accessioned | 2008-06-27T14:15:18Z | |
| dc.date.available | 2008-06-27T14:15:18Z | |
| dc.date.issued | 2002 | |
| dc.identifier.citation | Hartley , L E , Drew , J E & Long , K S 2002 , Time-resolved HST UV echelle spectroscopy of IX Vel . in In: The Physics of Cataclysmic Variables and Related Objects - ASP Conf Series 261 . Astronomical Society of the Pacific , pp. 483-484 . | |
| dc.identifier.isbn | 978-1-58381-597-7 | |
| dc.identifier.isbn | 1-58381-101-X | |
| dc.identifier.other | PURE: 151262 | |
| dc.identifier.other | PURE UUID: a2932ccb-d9fe-45e9-86ac-a8617d216722 | |
| dc.identifier.other | dspace: 2299/2153 | |
| dc.identifier.uri | http://hdl.handle.net/2299/2153 | |
| dc.description | Original paper can be found at: http://www.astrosociety.org/pubs/cs/253.html Copyright ASP | |
| dc.description.abstract | In the hydrodynamical line-driven disk wind models of Proga, Stone & Drew (1998) the mass loss rate is a strong function of the local luminosity. Also, the outflow is found to be subject to clumping, where the main source of driving radiation is the accretion disk. In order to test these predictions, we have obtained high resolution UV spectroscopy of the brightest novalike variable, IX Vel. These data have allowed us to examine the line profile structure in unprecedented detail. | en |
| dc.language.iso | eng | |
| dc.publisher | Astronomical Society of the Pacific | |
| dc.relation.ispartof | In: The Physics of Cataclysmic Variables and Related Objects - ASP Conf Series 261 | |
| dc.title | Time-resolved HST UV echelle spectroscopy of IX Vel | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
