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MisV0701     Profile MisV0701 = V1511 Aql R.A. 19h00m31s.77 Decl. -02o12'20".4 (2000.0) Mag. 13.0-14.8C Type SR = USNO-A2.0_0825.14008002 19 00 31.767 -02 12 20.35 14.7R 19.3B = IRAS 18579-0216 R.A.=19 00 34.05 Decl.=-02 12 01.7 (19 x 6", p.a. =81) flux(12)=3.98 flux(25)=15.99 flux(60)=7.45 flux(100)=<83.72 29% 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. Taichi Kato pointed out that this object is identified with a planetary nebula PK32-3.1. The catalogued position of PK32-3.1 is 47 arcsec from MisV0701. Special Notes Taichi Kato pointed out that it is near by a planetary nebula PK 32-3.1 and influenced to the past observations of PK 32-3.1. MISAO's observations, followed by TASS's observations, revealed that MisV0701 is a red variable. In the past papers (Stenholm & Acker, MacConnell), PK 32-3.1 was noted that maybe it is not a planetary nebula because the spectrum was that of a red variable. But the spectrum was probably the mixture with a red variable MisV0701. The IRAS data is on the border between a planetary nebula and a red variable. That is probably the mixture of the two objects' characteristics, too. Research and Publication MisV Stars in the TASS Tenxcat Database Yoshida, S.; Richmond, M. Influence of MisV0701 to a planetary nebula PK 32-3.1 Yoshida, S.; Kadota, K.; Kato, T.; Richmond, M. Light Curve MisV Stars in the TASS Tenxcat Database Yoshida, S.; Richmond, M. Observations by MISAO Project Date Mag Filter Observer 1999 Apr. 14.76013 13.2 C Ken-ichi Kadota 1999 Apr. 14.76057 13.1 C Ken-ichi Kadota 1999 May 8.71331 13.0 C Ken-ichi Kadota 1999 May 8.71374 13.1 C Ken-ichi Kadota 1999 July 24.51586 14.8 C Ken-ichi Kadota 1999 July 24.51653 [14.6 C Ken-ichi Kadota