Abstract
A deep (R ∼ 19.5) photographic Hα Survey of the southern Galactic Plane was recently completed using the UK Schmidt Telescope at the AAO. In addition, we have recently started a similar, CCD-based survey of the northern Galactic Plane using the Wide Field Camera on the INT. Both surveys aim to provide information on many types of emission line objects, such as planetary nebulae, luminous blue variables and interacting binaries. Here, we focus specifically on the ability of Hα emission line surveys to discover cataclysmic variables (CVs). Follow-up observations have already begun, and we present initial spectra of a candidate CV discovered by these surveys. We also present results from analyzing the properties of known CVs in the Southern Survey. By calculating the recovery rate of these objects, we estimate the efficiency of Hα-based searches in finding CVs.
Original language | English |
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Title of host publication | Interacting binaries accretion, evolution, and outcomes American institue of physics conference proceedings |
Place of Publication | Woodbury. NY |
Publisher | American Institute of Physics |
Pages | 643-646 |
Number of pages | 4 |
Volume | 797 |
ISBN (Print) | 0735402868, 9780735402867 |
DOIs | |
Publication status | Published - 21 May 2005 |
Event | Interacting binaries: accretion, evolution, and outcomes - Cefalu, Sicily, Italy Duration: 4 Jul 2004 → 10 Jul 2004 |
Other
Other | Interacting binaries |
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Country/Territory | Italy |
City | Cefalu, Sicily |
Period | 4/07/04 → 10/07/04 |
Keywords
- Cataclysmic variables
- Galactic surveys
- Ha
- Interacting binaries