[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-chat 3985] Re: (fwd) V445 Pup (Eyres)
- Date: Wed, 17 Jan 2001 22:25:08 +0900 (JST)
- To: vsnet-campaign-nova, vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 3985] Re: (fwd) V445 Pup (Eyres)
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Re: (fwd) V445 Pup (Eyres)
> A number of symbiotic stars, particularly the so-called symbiotic
> novae (e.g. HM Sge) have spectra early in their outbursts which show
> no hint of a red giants, and often these objects were not even
> identified as symbiotic stars until outburst. Also, as far as I can
> tell some symbiotic novae (e.g. HM Sge, V1016 Cyg) do not appear in
> the 2MASS Second Incremental Release Point Source Catalog. The
> H-deficiency is harder to explain in the symbiotic model however.
They are very bright 2MASS sources.
HM Sge:
2MASS 194157.072 +164439.48 (2000.0) 0.000 0.000 0.000
2MASS 194157.072 +164439.84 (2000.0) 0.000 0.000 0.000
2MASS 194157.086 +164439.85 (2000.0) 7.619 6.011 4.652
V1016 Cyg:
2MASS 195705.030 +394936.33 (2000.0) 7.017 5.794 4.721
2MASS 195705.064 +394935.76 (2000.0) 0.000 0.000 0.000
Regards,
Taichi Kato
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp