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[vsnet-chat 4572] Re: new Tycho variables...
- Date: Sat, 30 Jun 2001 21:12:13 -0300
- To: <crawl@zoom.co.uk>, <vsnet-newvar@kusastro.kyoto-u.ac.jp>, <vsnet-chat@kusastro.kyoto-u.ac.jp>
- From: "Sebastian Otero" <varsao@sinectis.com.ar>
- Subject: [vsnet-chat 4572] Re: new Tycho variables...
- References: <3.0.6.32.20010630124554.00797810@pop3.zoom.co.uk>
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
> A list of freshly analysed possibly variable stars from the Tycho data
> annexes can be found at the CDS ftp site under the J/A+A/373/576
subdirectory.
> of the
> potentially variable objects that he also lists in newvar.cat, several of
> the Luminous Milky Way stars are suggested to be variable according to
this
> fresh analysis of Tycho Epoch Photometry.
>
> List follows:-
John and all:
I have searched for photometry (from GCPD) of these stars
and I don't think that something worth can be done visually. Furthermore I
have my doubts regarding some of them being actually variable!
One by one:
> > LSV+55.2 3690 1948 1 1069
ID / V, B-V from all PEP sources
HD 901 / 7.43, 1.26 ; 7.437, 1.279 ; 7.43
it looks very constant!!!!! Even Hipparcos V magnitude is 7.43.
> > LSV+57.33 3694 1727 1
BD +56 618
No data
> > LSI+61.282 4046 118 1
BD +60 501 / 9.51, 0.45 ; 9.58, 0.44 ; 9.58, 0.45 ; 9.58 ; 9.60, 0.46 ;
9.60
> > LSV+35.12 2402 6 1 2517
HD 2841 / 6.885
Hipparcos magnitude is 6.87. B-V is 1.64.
> > LSII+27.26 2148 3858 1
HD 333048
No data
> > LSIII+55.25 3973 1031 1
HD 235749 / 8.81, 1.71 ; 8.93, 1.60
This one seems to be an ordinary red variable deserving attention !!!
> > LSIII+47.58 3611 701 1 11092
HD 14606 / 7.684, 0.198
And Hipparcos V magntiude is 7.69. Doubtful...
> > LSI+59.24 4281 2033 1
HD 240464 / 9.583; 9.59, 0.30 ; 9.59, 0.31 ; 9.62, 0.32
Doesn't seem to be...
> > LSS4360 6840 821 1 8689
HD 11326 / 6.589 ; 6.595 ; 6.606
Hipparcos V magnitude 6.59, B-V 1.10. It also looks constant.
> > LSS4857 6269 2398 1
HD 167611 / 9.45, 0.19 ; 9.450 ; 9.481 ; 9.52, 0.16
This one looks slightly variable.
Regards,
Sebastian.
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