[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]

[vsnet-newvar 1377] New variable star MisV1159

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1159).

MisV1159
  R.A.  21h15m14s.07
  Decl. +49o54'10".3  (2000.0)
  Mag.  13.3-15.6C
  Type  M?
= IRAS 21135+4941  21h15m14s.1 +49o54'08"  Ellipse:8x5"  P.A.:177  Flux(12):1.104  Flux(25):0.5421  Flux(60):<2.523  Flux(100):<25.73  Var:33%
= MSX5C G091.5023+00.7030  21h15m14s.30 +49o54'08".6  InScanError:2.8"  CrossScanError:1.5"  Flux(A):0.50921
= 2MASS 211514.033 +495409.78 (2000.0)  8.628  7.072  6.229

  http://vsnet.aerith.net/misao/data/MisV/MisV1159.gif

MisV1159 20000902.50517 14.20C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1159 20000902.50701 14.15C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1159 20000902.50887 14.39C Mis KAF-1600L Tycho-2_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1159 20001013.45255 13.26C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1159 20001013.45440 13.24C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1159 20011003.47015 15.57C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1159 20011003.47212 14.84C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1159 20011003.47410 14.91C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, MISAO Project, discovered a new variable star
MisV1159.

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, and confirmed by KenIchi Kadota. 

The identification is researched by Taichi Kato (Kyoto University),
John Greaves (the United Kingdom), and Seiichi Yoshida.

The magnitude are measured automatically by the PIXY system 2.

About the MISAO Project and the PIXY system 2:
  http://vsnet.aerith.net/misao/

--
Seiichi Yoshida
comet@aerith.net
http://vsnet.aerith.net/

VSNET Home Page

Return to Daisaku Nogami

vsnet-adm@kusastro.kyoto-u.ac.jp