Three new long-period CVs from the Hamburg Quasar Survey
UNSPECIFIED (2005) Three new long-period CVs from the Hamburg Quasar Survey. In: Conference on Astrophysics of Cataclysmic Variables and Related Objects, JUL 11-16, 2004, Strasbourg, FRANCE.Full text not available from this repository.
We present time-resolved optical spectroscopy and photometry of three new relatively bright (V similar to 14.0 - 15.5) long-period cataclysmic variables discovered in the Hamburg Quasar Survey: HS 0139+0559, HS 0229+8016 and HS 0506+7725. The orbital periods, 243.2 +/- 0.4 min, 233 +/- 1 min and 212.6 +/- 0.1 min, are determined from radial velocity studies. The light curve of HS 0506+7725 is characterised by flickering. HS 0229+8016 and HS 0139+0559 display practically no photometric variability. Whereas HS 0506+7725 is a weak X-ray emitter in the ROSAT All Sky Survey, HS 0229+8016 and HS 0139+0559 were not detected. The identification of these three systems underlines that the currently known sample of CVs is likely incomplete even for bright systems.
|Item Type:||Conference Item (UNSPECIFIED)|
|Subjects:||Q Science > QB Astronomy|
|Series Name:||ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES|
|Journal or Publication Title:||Astrophysics of Cataclysmic Variables and Related Objects|
|Publisher:||ASTRONOMICAL SOC PACIFIC|
|Editor:||Hameury, JM and Lasota, JP|
|Number of Pages:||2|
|Page Range:||pp. 469-470|
|Title of Event:||Conference on Astrophysics of Cataclysmic Variables and Related Objects|
|Location of Event:||Strasbourg, FRANCE|
|Date(s) of Event:||JUL 11-16, 2004|
Actions (login required)