[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-chat 3107] NSV02872
- Date: Sun, 18 Jun 2000 20:59:41 +0900 (JST)
- To: vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 3107] NSV02872
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
NSV02872
NSV02872 was originally discovered as a possible UG-type variable.
Recent studies have shown the candidate is a late-type star, which seems
to preclude the UG-type variability. However, I have noticed the following
ROSAT source close to the variable's position.
061408.2 +453029 (2000.0) 1RXS-F_J061408.3+453030 0.033 0.54 0.64
This possible association may suggest that the existence of the true
dwarf nova (or some eruptive variable) hidden in the glare of a red star.
This variable should deserve further attention.
Regards,
Taichi Kato
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
VSNET Home Page