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MisV1105 = V2421 Cyg
= GSC 3159-01247 20h14m38s.55 +41o56'14".6 Error:0.2" Mag:13.93 Ma gError:0.38 Band:1 Class:3 Plate:003S Flag:F Epoch:03 SEP 1983 = USNO-A2.0 1275.13699980 20h14m38s.575 +41o56'14".67 Mag(R):14.4 M ag(B):14.6
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and Ken-ichi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1105.
It was picked up by Seiichi Yoshida from the candidates of new variable stars detected by the PIXY system 2 from images taken by Nobuo Ohkura comparing with images taken by Ken-ichi Kadota, and confirmed by Ken-ichi Kadota.
The identification is researched by Taichi Kato (Kyoto University), John Greaves (the United Kingdom), and Seiichi Yoshida.
Kazuhiro Nakajima's observations revealed it is a beta Lyr-type (EB) eclipsing variable with unfiltered CCD variations of 13.79 mag at maximum, 15.03 mag at primary minimum, 14.20 mag at secondary minimum, and period of 0.6331 days (IBVS 5600).
Research and Publication
MisV1105 is a beta Lyr-type eclipsing variable
Nakajima, K.; Yoshida, S.; Ohkura, N.; Kadota, K.
Observations by MISAO Project