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MisV0562     Profile MisV0562 R.A. 18h41m16s.71 Decl. -29o04'41".7 (2000.0) Mag. 11.9-13.6V Type SR Period 320 Epoch 2452070 = GSC6870.1256 18 41 16.82 -29 04 40.5 12.95 = USNO-A2.0_0600.36576635 18 41 16.707 -29 04 41.74 12.2R 17.4B = IRAS 18380-2907 R.A.=18 41 13.36 Decl.=-29 04 43.5 (74 x 9", p.a. =86) flux(12)=1.57 flux(25)=0.87 flux(60)=<0.40 flux(100)=<1.33 0% variable Digitized Sky Survey GIF image (15 x 15 arcmin) SIMBAD Query AAVSO VSX Database ASAS-3 Light Curve Discovery Information It was detected by the PIXY system as one of the candidates of new variable stars from images taken by Ken-ichi Kadota, Ageo City, Saitama, Japan, then confirmed by Seiichi Yoshida. Special Notes Mati Morel pointed out the possible identification with Luyten's V915 Sgr. The range by Luyten (12.3-13.5p) is not too dissimilar to that of MisV0562 (11.8-13.8C). V915 Sgr is regarded as GSC 6870-00090 in Herbig's paper (PASP 70,605) and classified as RCB type with a period of 285.2 days, which can well refer to the period of MisV0562. If MisV0562 is V915 Sgr, it turns out to be a SR variable [vsnet-chat 2797]. However, the variability of V915 Sgr = GSC 6870-00090 was also detected in the MISAO Project. So MisV0562 is a new variable star [vsnet-chat 2803]. Light Curve Light curve by ASAS-3 observations Copyright (C) Grzegorz Pojmanski / The All Sky Automated Survey Light curve by ASAS-3 observations Copyright (C) Grzegorz Pojmanski / The All Sky Automated Survey Observations by MISAO Project Date Mag Filter Observer 1999 July 15.58797 13.8 C Ken-ichi Kadota 1999 July 15.58841 13.5 C Ken-ichi Kadota 1999 Sept. 23.44072 11.8 C Ken-ichi Kadota 1999 Sept. 23.44116 11.8 C Ken-ichi Kadota