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http://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/14209Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Vaidya, Kaushar | - |
| dc.date.accessioned | 2024-02-12T06:28:02Z | - |
| dc.date.available | 2024-02-12T06:28:02Z | - |
| dc.date.issued | 2006 | - |
| dc.identifier.uri | https://iopscience.iop.org/article/10.1086/499206/meta | - |
| dc.identifier.uri | http://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14209 | - |
| dc.description.abstract | We present cross-identification of archived ROSAT X-ray point sources with W UMa variable stars found in the All-Sky Automated Survey. A total of 34 W UMa stars have been found associated with X-ray emission. We compute the distances of these W UMa systems and hence their X-ray luminosities. Our data support the "supersaturation" phenomenon seen in these fast rotators, namely that the faster a W UMa star rotates, the weaker its X-ray luminosity. | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | IOP | en_US |
| dc.subject | Physics | en_US |
| dc.subject | ROSAT X-ray point | en_US |
| dc.subject | W UMa variable | en_US |
| dc.subject | X-ray luminosity | en_US |
| dc.title | W Ursae Majoris Contact Binary Variables as X-Ray Sources | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | Department of Physics | |
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