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[vsnet-alert 5106] Re: Sequences near LMC nova



There is a lot more UBV data for field stars near the LMC nova, but it
usually involves digging through old papers. A compiled sequence of stars is
presented below, but has been done in a hurry, so excuse me if references
are not so complete.

LMC Nova 2000. Sequence.
====================
Name          HDE         V    B-V       RA  (2000)  DEC.
======================================
                 269451    12.56  -0.05  5:22:20.3 -70:36:06
                 269510    11.11 +0.22  5:25:08.2 -69:53:44
                 269584    10.83 +0.52  5:27:31.6 -70:26:27
NS-70o91                12.78  -0.23  5:27:33.8 -70:36:48
NS-70 93 269585    12.84 +0.07  5:27:48.7 -70:07:27
NS-70 94                 13.13: -0.14  5:28:57.9 -70:20:29

These are LMC B or A type supergiants, and the same data is (or should be)
in the Geneva Catalogue of Photometric Data.
Other useful BV data comes from the work on foreground stars by Gochermann,
Grothues et al, as follows.

FD 989   269505     10.92 +0.43  5:24:56.2  -70:16:11   GSC 9166.178
FD 1000 269520     10.24 +0.97  5:25:26.1  -70:11:35
                                11.67 +0.56  5:25:45.3  -70:05:44   GSC
9166.556
                                11.84 +0.62  5:26:52.1  -70:12:55   GSC
9166.30

Sorry, no time to find all other aliases for the ids  NS = N. Sanduleak.
Ref:  Gochermann, J., Grothues H-G., Oestreicher M.O., Berghoefer T.,
Schmidt-Kaler  T.
Astron. Astrophys. Suppl. 99,591 (1993).

This particularly region of the LMC is especially prolific for novae. Within
a 1degree radius of the
new nova, other novae have appeared in  1948, 1970 (2 novae), 1981, 1987 and
1988, that  I know of.
I haven't got a complete census at the present moment.
Cheers, Mati

Morel Astrographics
c/o M. Morel, 6 Blakewell Rd, Thornton NSW 2322 AUSTRALIA
*Specialized Charts** Variable Star Studies** Stellar Data**
151o38'33" E, 32o46'47"S.               morel@ozemail.com.au
----- Original Message -----
From: Brian Skiff <bas@lowell.edu>
To: <vsnet-alert@kusastro.kyoto-u.ac.jp>
Sent: Friday, July 14, 2000 9:23 AM
Subject: [vsnet-alert 5103] Sequences near LMC nova


>      Here are two sequences near the new LMC nova.  Both are however about
> 50' away.  Perhaps Mati Morel knows of some stars closer to the object.
>
> \Brian
>
>
>
> Name                  RA  (2000)  Dec        GSC       V    B-V
> Martin LMC III-1    5 14 37.0  -70 13 20  9166-0172  11.84  0.77
> Martin LMC III-2    5 14 59.3  -70 11 17  9166-0404  12.43  0.69
> Martin LMC III-3    5 14 27.5  -70 11 34             14.98  0.87
> Martin LMC III-4    5 15 04.6  -70 09 41             15.15  0.16
> Martin LMC III-5    5 15 05.0  -70 11 45             15.82  0.93
>
> NGC 2058 W          5 36 28.1  -70 17 47  9167-0391  10.43  0.54
> NGC 2058 E          5 36 53.2  -70 07 44  9167-0516  11.93  0.93
> NGC 2058 D          5 36 36.8  -70 07 16  9167-0485  12.39  0.67
> NGC 2058 F          5 36 39.8  -70 09 28  9167-0806  12.52  0.55
> NGC 2058 K          5 37 19.3  -70 18 07  9167-0772  12.94  0.97
> NGC 2058 H          5 35 30.7  -70 14 45  9166-0658  13.06  0.56
> NGC 2058 V          5 37 18.7  -70 13 37             13.19 -0.08
> NGC 2058 S          5 36 57.2  -70 20 03             13.67  0.63
> NGC 2058 A          5 36 56.2  -70 05 14             13.77  0.41
> NGC 2058 C          5 36 48.8  -70 13 18             13.83  0.50
> NGC 2058 J          5 36 31.5  -70 09 05             14.16  0.63
> NGC 2058 T          5 37 02.1  -70 21 32             14.17  0.58
> NGC 2058 Y          5 37 17.5  -70 13 50             15.36  0.74
>

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