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[vsnet-chat 3125] Re: (fwd) Re: LMC V1341 prelim sequence (Greaves)
- Date: Wed, 21 Jun 2000 22:43:26 +1000 (EST)
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: Mati Morel <morel@ozemail.com.au>
- Subject: [vsnet-chat 3125] Re: (fwd) Re: LMC V1341 prelim sequence (Greaves)
- Cc: crawl@zoom.co.uk
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
At 09:48 AM 6/21/00 +0900, you wrote:
>(fwd) Re: LMC V1341 prelim sequence (Greaves)
>
>From: crawl@zoom.co.uk
>Date: Tue, 20 Jun 2000 17:25:31 +0000
>Subject: re [vsnet-chat 3114] Re: LMC V1341 prelim sequence
>
>Hi All & Mati
>
>The tables in data format for A+AS 121, 247 can be downloaded via :-
>
>http://cdsarc.u-strasbg.fr/cats/J/A+AS/121/247/
>
>whilst A+AS 99, 591 lives at:-
>
>http://cdsarc.u-strasbg.fr/cats/J/A+AS/99/591/
>
[snip]
>Sideways : I note that the USNO derived colour for GSC 9169 1555 is
>totally contradictory to the B-V you quote for the same object, Mati :
>are you sure of the ID...?
>
>John
Hi John and others,
The star GSC 9169 1555 is also known as HDE 271060, sp. type K7. So, the UBV
colours
B-V +1.56 U-B +1.83 are quite consistent with that spectral class. I see no
problem
with id.
The only problem I see is with the range of V1341 : 10.9 -15.7p. This is not
credible
for your typical Recurrent Nova. Maybe the figure 15.7 refers to a field
star about
40 arcsec to the south. At the distance of the LMC one would not expect any
novae to be
visible at quiescence.
Cheers,
Mati
/Mati
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