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[vsnet-chat 2644] NSV4223 Pyxidis
- Date: Mon, 7 Feb 2000 18:16:29 +0800
- To: <vsnet-chat@kusastro.kyoto-u.ac.jp>
- From: "Andrew Pearce" <arpearce@ozemail.com.au>
- Subject: [vsnet-chat 2644] NSV4223 Pyxidis
- Cc: <b.sumner@bom.gov.au>, <tkato@kusastro.kyoto-u.ac.jp>, <varstar@voyager.co.nz>
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
I have been observing the suspected variable NSV4223 in Pyxis over the last 40
days or so. During this time I have detected quite a large drop in brightness
amounting to nearly 3 magnitudes as indicated in the observations below:
JD Mag
2451541.2938 10.4
2451544.2813 10.4
2451547.2674 10.4
2451576.2639 11.9
2451577.2604 12.3
2451579.2674 13.0
2451580.2882 13.0
2451581.2611 13.2
The VSS of RASNZ has a chart for this star (Chart No. 1122) with letter
designation for comparison stars as a proper sequence is not available. I have
assigned magnitudes to these stars based on the Tycho Johnson V mags for the
brighter stars and GSC mags for stars fainter than 11th mag. The GSC magnitudes
appear to be suspect with most of them appearing to be on the faint side of what
the comparison stars actually appear.
In any case it appears that the object's variability is beyond question. I note
that it's spectral type is listed as SE.
I would be interested to hear if anyone else has observed this star and if there
are any reports on the type of star it actually is.
I will keep on observing the star, and I urge others to as well, so we can get a
better idea of it's light curve.
Regards
Andrew Pearce
Western Australia
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