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Var Psc

MUY
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Joined: 2010-07-23

Hi,

The suspected UG-variable Var Psc is not in the VSX. Is there more information known about this star? Has it been dropped as a probable dwarf nova?

There is a sequence for this star (and RZ Psc), made by Bruce Sumner :

http://joevp.20m.com/charts/henden/Her%20to%20Vul/Psc_Var.txt

 

Thanks,

Eddy (MUY)

 

var Psc 2010
pukemaru
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Hi Eddy

Do you mean var Psc 2010? at 23h 04m 26s   +06° 25’ 45”, UG   11.5 – 21 CR.

If so, just type in var Psc 2010. It is in VSX but there is no sequence. I use a sequence by Mati Morel Chart 66-A00028.

Interestingly, when I searched WebObs, I found the star listed as SDSS J230425.87+062545.7 with 17 observations all by you.

Kind regards, Stephen [HSP]

Var Psc
MUY
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Hi Stephen,

Yes, I have SDSS J230425.87+062545.7 (Var Psc 2010) on my observing list but Var Psc is another suspected CV. Here is a chart with the coordinates :

http://joevp.20m.com/cgi-bin/i/charts/henden/Her%20to%20Vul/Psc_Var_C_reverse.jpg

Regards,

Eddy

var Psc
pukemaru
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Hi again, Eddie. Thanks for the chart. It's a bit far north for me although I do observe AW Gem occasionally and that's +28.

I did a coordinate search in VSP and voilá, found  EQ J010959.2+280125

That is your star and it's listed in VSX under this name. There are 4 references in VSX.

Kind regards

Stephen

Var Psc
MUY
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Joined: 2010-07-23

Hi again Stephen,

The reason I didn't find it is because I was searching in the list with cataclysmic variables.  I see that it's no longer a CV... The VSX gives non-cv. According Downes it's a F-type star.

Cheers,

Eddy

Var Psc
PYG
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Joined: 2010-07-08

It's in the same field as the UXOR star RZ Psc, so why not estimate it at the same time?  You never know what Var Psc might get up to.  I have years of data on it, and it certainly isn't a flat line light curve.  Small amplitude variations maybe, but it's not steady. 

Gary [PYG]

Var Psc
HQA
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Joined: 2010-05-10

Hi Gary,

The CRTS light curve shows about 0.1mag variations, so it is probably below the measurement level of most visual observers.  APASS gives (B-V) = 0.5, as did my USNO measurements, in agreement with the F-classification from Downes.  While estimating it because it is in the field of RZ Psc makes some sense, I would not make this a high priority estimate.  Perhaps some of the time-series folks who have looked at RZ Psc have higher time resolution datasets that could pin down whether this is a periodic variable, a chaotic one, or not variable at all.

Arne

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