MISAO Project

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    MisV0701    

* Profile

MisV0701 = V1511 Aql

R.A.19h00m31s.77
Decl.-02o12'20".4(2000.0)
Mag.13.0-14.8C
TypeSR
= 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

* Light Curve


MisV Stars in the TASS Tenxcat Database
Yoshida, S.; Richmond, M.

* Observations by MISAO Project

DateMagFilterObserver
1999 Apr. 14.7601313.2CKen-ichi Kadota
1999 Apr. 14.7605713.1CKen-ichi Kadota
1999 May 8.7133113.0CKen-ichi Kadota
1999 May 8.7137413.1CKen-ichi Kadota
1999 July 24.5158614.8CKen-ichi Kadota
1999 July 24.51653[14.6CKen-ichi Kadota

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