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[vsnet-chat 1709] Re: [AAVSO-DIS] DHK 42 TAU
- Date: Mon, 29 Mar 1999 12:44:34 +0900 (JST)
- To: aavso-discussion@physics.mcmaster.ca
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 1709] Re: [AAVSO-DIS] DHK 42 TAU
- Cc: vsnet-chat
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
> I'm sure the discoverer will chime in here, but SIMBAD shows that this
> star is a mid-M star, so presumably a Mira, located in the background of the
> Hyades cluster. DHK 42 = V1100 Tau = IRAS 04184+2008 = StM 33.
Other identifications:
GSC1272.567 042125.33 +201559.4 (2000.0) 14.30 1
GSC1272.567 042125.45 +201558.6 (2000.0) 14.44 1
USNO1050.01252584 042125.409 +201558.95 (2000.0) 10.0 13.6
042125.1 +201559 (2000.0) LMS33 M6 >13.5
042125.3 +201558 (2000.0) Q1993/009 10.9 <12.0
042125.6 +201559 (2000.0) IRAS04184+2008 16.000 5.225 0.950 1.696L 99%
042125.6 +201559 (2000.0) SSC04184+2008 16.000 5.225 0.950 1.696L
042126.0 +201559 (2000.0) FSC04185+2008 12.370 4.840 0.923 4.467L
042125.3 +201558 (2000.0) TAUV1100 M 12.5 (15.5 P - - - -
042125.9 +201703 (2000.0) WSV15
The last entry (WSV15) shows that this variable was independently discovered
by M. Wakuda.
Regards,
Taichi Kato
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