[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-chat 3982] (fwd) Re: Nc's and other peculiar variables (Bedient)
- Date: Wed, 17 Jan 2001 18:30:36 +0900 (JST)
- To: vsnet-campaign-nova, vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 3982] (fwd) Re: Nc's and other peculiar variables (Bedient)
- Cc: aavso-discussion@informer2.cis.McMaster.CA
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
(fwd) Re: Nc's and other peculiar variables (Bedient)
Date: Tue, 16 Jan 2001 22:59:19 -1000
From: Jim Bedient <bedient@amsmeteors.org>
Subject: Re: [vsnet-campaign-nova 167] Re: Nc's and other peculiar
variables
At 04:45 PM 1/17/01 +0900, Taichi Kato wrote:
>Symbiotic stars usually
>have red giants, whose signature could have been easily detected by the
>2MASS survey, but the possibility is rather unlikely becuase of the
>relatively blue color of the progenitor.
There is a 2MASS point source very close to the position reported in IAUC
7556 by Platais et al. for V445 Pup (R.A. = 7h37m56s.882, Decl. =
-25o56'58".88 (J2000)). 2MASSI J0737568-255658 is listed at R.A. = 07h 37m
56m.881, Decl. = -25o 56' 58".85 (J2000) in the Two Micron All Sky Survey
(2MASS) Second Incremental Data Release Point Source Catalog.
Assuming the two objects are one and the same, the following photometric
magnitudes from the 2MASS Second Incremental Data Release Point Source
Catalog represent pre-outburst observations of V445 Pup (epoch 1999 Feb.
2.236): J = 12.270 +/- 0.031, H = 11.933 +/- 0.036, K = 11.515 +/- 0.030.
J. Bedient
Honolulu, Hawaii
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp