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[vsnet-chat 2309] Re: GM Sgr
- Date: Fri, 17 Sep 1999 09:13:02 -0700
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: aah@nofs.navy.mil
- Subject: [vsnet-chat 2309] Re: GM Sgr
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
I notice that IAUC 7253 (which we just got in today;
the circulars first go to USNO-DC and then sometime later,
often a week later, we get to see them) gives the
coordinates as measured by Gareth to +/- one arcsec.
I think they are better than that in Sumner's sequence file:
http://ftp.nofs.navy.mil/pub/outgoing/aah/sequence/sumner/gmsgr.seq
(several measurements vs. USNO-A2.0).
Also, the circular implies that Luyten and Goranskij looked
at the same star. Someone should put in a clarification.
Looking at the ASM light curve, there appears to be
a 20-hour delay between the optical peak and the later
X-ray burst. Is there an explanation for this? The flux
curve shapes are not as similar as I would have expected. The
combined light curve also suggests that the V=8.8 was not
the actual peak, which might have occurred several hours
earlier. That would have been interesting to see!
Arne
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