[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-chat 3134] OV Tau
- Date: Thu, 22 Jun 2000 13:08:17 +0900 (JST)
- To: vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 3134] OV Tau
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
OV Tau
Another case of noteworthy CV candidate - ROSAT identification.
OV Tau:
USNO1125.01275716 034606.260 +294114.69 (2000.0) 14.3 15.9
034606.2 +294114 (2000.0) 15.47 0.78 Henden
034606.2 +294114 (2000.0) TAUOV * UG 15.5 16.5 P - 7.5 - pec(cont+e) R0/DOW
ROSAT:
034605.8 +294117 (2000.0) 1RXS-F_J034605.9+294118 0.035 1.00 0.43
The identification seems to be secure. OV Tau was originally regarded
as a dwarf nova, but was dropped from the CV list based on spectroscopy
(detached binary). The present ROSAT identification probably cast a
new light on this problem. The ROSAT spectrum sounds too hard for
a non-accreting white dwarf. Is X-ray from the companion?
Regards,
Taichi Kato
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp