[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-chat 3318] re NSV14667 = ASAS_J234131+0126.4
- Date: Sat, 01 Jul 2000 14:09:59 +0000
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: no name <crawl@zoom.co.uk>
- Subject: [vsnet-chat 3318] re NSV14667 = ASAS_J234131+0126.4
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Taichi Kato wrote:
> Another possible ROSAT identification with an ASAS variable.
> The period of 7.45d is long for a dK2 star (what type is expected?)
If you looked at the folded light curve on
http://archive.princeton.edu/cgi-asas/asas_variable/234131+0126.4,7.450892
you'd think Cepheid...
...but I think the very noisy and seriously gapped raw light curve tells
the true story...
[gapped data which has an increasing trend at one side and a declining
trend on the other can do this sort of trick. I once made the same
mistake myself on a highly seasonal symbiotic star (I forget which one)
using visual data. I got a very quasi-sinusoidal result!
Further, I've just PDMed the data from the website, and you can get a
pretty good 0.2 I amplitude folded curve of 1.152 day period of theta
statistic 0.58 (and by eye you can still "find" smaller ripples in
that!)]
Cheers
John
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp