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    MisV1095 is an Algol-type eclipsing variable    

October 11, 2003
Nakajima, K.; Yoshida, S.; Ohkura, N.

Kazuhiro Nakajima revealed that MisV1095 is an Algol-type eclipsing variable with unfiltered CCD variations of 12.64 mag at maximum, 13.24 mag at primary minimum, 12.90 mag at secondary minimum, and period of 1.5829 days.

MisV1095, R.A. 00h26m49s.46, Decl. +41o49'08".9 (J2000.0), is a new variable star discovered in the course of the MISAO Project from Nobuo Ohkura's unfiltered CCD images taken between Sept. 20 and Nov. 6 in 2000.

Nakajima observed it on 6 nights between Sept. 5 and 17 in 2003 with 0.25-m f/5 Schmidt-Cassegrain and CV-04 CCD, and caught four minima.

MinimumHJDError of HJD

The period is derived as 1.5829 days from these minima.

Here is the light curve of MisV1095 from total 463 observations. Comparison star is TYC2-2791.2222.1, R.A. 00h26m04s.0, Decl. +41o48'00" (2000.0), 11.09 mag(V). The phases on the figure were calculated by the ephemeris:

Primary minimum HJD = 2452900.1019 + 1d.5829 x E

[vsnet-newvar 2246]

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