VSX : Detail for GSC 04015-00167

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Name

GSC 04015-00167

AAVSO UID

000-BKQ-602 (20422 observations)

Constellation

Cassiopeia

Sequence

J2000.0

00 22 26.52 +61 49 39.7 (5.61050 +61.82769)

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B1950.0

00 19 41.44 +61 33 01.7

Proper motion

RA: -3.837 +/- 1.058 mas/y

Dec: -0.295 +/- 0.759 mas/y

Source: Gaia DR1

Galactic coord.

119.516 -0.852

Other names

(Internal only)

2MASS J00222651+6149398	ALS 6158	ASASSN-V J002226.36+614940.2
LS I +61 145	TYC 4015-167-1	USNO-B1.0 1518-0012060
VSX J002226.5+614939

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Variability type

Spectral type

B1V

Mag. range

11.206 - 11.305 CV

Discoverer

Enrique de Miguel (CBA, Spain)

Epoch

14 Sep 2010 (HJD 2455453.549)

Ephemeris

Outburst

Period

1.84628 d

Rise/eclipse dur.

12% (5.3 h)

Remarks

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de Miguel , Enrique

The star shows total eclipses, the CV magnitude of the secondary eclipse being 11.229. The light curve exhibits reflection effect. Assuming the orbital to be circular with inclination i =90º, the radii of the primary (1) and secondary (2) stars are approximately given by R1/a= 0.28 and R2/a= 0.09, with a being the binary separation. The distance is estimated as 4.03+/- 0.66 kpc, according to Russeil et al., A&A 470, 161 (2007).

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References

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Location

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Catalog Data

Information from selected catalogs obtained by cross-matching to 2 arc seconds using the CDS X-Match Service. These data may not be complete.

2MASS	J = 10.77	H = 10.75	K = 10.74	J - K = 0.03
AllWISE	W1 = 10.72	W2 = 10.77	W3 = 9.52	W4 = 5.56	W1 - W2 = -0.05	W3 - W4 = 3.96
APASS-DR9	B = 11.39	V = 11.17	g' = 11.26	r' = 11.20	i' = 11.26	B - V = 0.23

Images

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Size	5' x 5' (297 x 298 pixels)
Center	00 22 26.52 +61 49 39.7 (J2000)
Source	STScI
Survey	Red, all sky, 1.0 arcsec/pixel
	Negative

Supporting Documents

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2	Phased light curve TYC 4015-167-1	de Miguel , Enrique	2012-09-09 03:06 UTC	Differential photometry carried out relative to TYC 4015-77-1 (APASS magnitude V=11.563). This eclipsing binary exhibits total eclipses.
1	Detail of the primary eclipse	de Miguel , Enrique	2012-09-09 03:06 UTC	Detail of the primary eclipse. First contact is estimated to occur at phase phi_1= - 0.063, and second contact at phase phi_2= - 0.030.