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[vsnet-chat 4509] Liller's var in LMC = LMC V2434
- Date: Fri, 8 Jun 2001 16:38:26 +1000
- To: <aavso-discussion@informer2.cis.mcmaster.ca>, <vsnet-chat@kusastro.kyoto-u.ac.jp>
- From: "Mati Morel" <morel@ozemail.com.au>
- Subject: [vsnet-chat 4509] Liller's var in LMC = LMC V2434
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
----- Original Message -----
Sent: Friday, June 08, 2001 2:26 P
Subject: Liller's var in LMC (with minor corrections).
> Hi All,
> Bill Liller's latest discovery in the LMC is a known variable,
with
> a fairly extensive history. It is LMC V2434. A potted history follows.
> K. Henize (ApJ Suppl 22, 1956) recorded it as S162 (emission line star).
He
> remarks : "Continuum appears reddish. Perhaps a late-type star?"
> Bohannon and Epps (1974) in their survey of LMC emission line stars,
record
> it as BE577.
> J.P. Brunet et al (Astron. Astrophys. Suppl. 21, 109-136, 1975) record it
as
> Brunet156, spectrum Be.
> R.M. Humphreys (ApJ Suppl39, 389-403, 1979), calls it Blanco72, a
foreground
> star and a long period variable. Data given:
> V = 12.90
> B-V = 1.47
> V-R = 1.68
> V-I = 3.24
> Spect.: M2e III
>
> Also known as Case 48-8. Humphreys notes it as a LPV with hydrogen and Ca
II
> H and K in emission.
>
> LMC V2434 = GSC 9166.00775 at (2000) 5h24m1.6s -71'35.6". Lies a
> little west of W Men, but a selection of closer comparison stars is given
> here.
> HDE RA 2000 DEC 2000 V B-V U-B Quality
> 269479 5:23:22.4 -71:05:34 10.59 0.41 -0.03 2
> ........... 5:23:22.0 -71:11:40 13.68 0.08 0.23 2
> 269488 5:23:43.8 -71:11:58 12.21 0.64 0.10 2
> ........... 5:23:49.1 -71:03:34 12.33 0.62 0.22 2
> 269493 5:24:01.7 -71:18:23 11.93 0.65 0.12 2
> 269495 5:24:12.8 -71:09:12 10.48 1.02 0.76 2
> 269498 5:24:23.3 -71:01:57 12.11 0.89 0.70 2
> 269507 5:24:47.9 -71:01:38 10.97 1.27 1.29 2
> ............ 5:25:17.1 -71:02:51 11.78 1.10 1.00 2
> 269538 5:25:57.0 -70:58:15 9.84 0.53 -0.01 2
>
> The pe data is taken from Gochermann et al ( A & A Suppl 99,591, 1993) and
> subsequent papers. The quality rating indicates more reliable data -2 or
> more obs. per star, as distinct from a rating of "1" (only one obs.)
>
> The data seems to indicate a Z And type star, yes? The magnitude of 9.8
> observed by Bill seems to be far outside the range previously observed for
> this star.
>
> Cheers,
> Mati
> ++++++++++++++++++++++++++++++++++
> Morel Astrographics
> *Charts*Variable Star Studies* Specialized charts*
> email: morel@ozemail.com.au
> Web: http://vsnet.ozemail.com.au/~morel
> ++++++++++++++++++++++++++++++++++
>
>
>
>
>
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