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[vsnet-newvar 295] New Haseda variable (HadV46)



New Haseda variable (HadV46)

   Katsumi Haseda (Aichi, Japan) reports the discovery of a new variable
star (HadV46).

   Although the light variation is not inconsitent with a Mira-type variable,
the examination by Haseda of the RealSky image confirms the identification
with

= USNO0750.13650086 183404.041 -144500.23 (2000.0) 14.4 15.5

   , which is not red as expected from the light variation.  More detailed
observation (multicolor photometry and possibly spectrocopy) would be
desired to clarify the nature of the object.  The object is bright now.

   There is an IRAS source an arcmin away,

183401.4 -144534 (2000.0) IRAS18311-1447 0.596 1.371L 7.393L 104.700L -1%

   but is more likely identified with a red star

USNO0750.13647965 183402.251 -144533.69 (2000.0) 11.6 16.7

HadV46
= USNO0750.13650086 183404.041 -144500.23 (2000.0) 14.4 15.5

  HadV46  ?  10.6-(13.3p

Photographic magnitude estimates by VSOLJ members

object         YYYYMMDD(UT)   mag  code
HadV46         19960525.676  126p  Had.VSOLJ
HadV46         19980816.522  <133p  Had.VSOLJ
HadV46         19981108.403  <133p  Had.VSOLJ
HadV46         19990219.822  <133p  Had.VSOLJ
HadV46         19990322.782  <131p  Had.VSOLJ
HadV46         19990831.483  <130p  Had.VSOLJ
HadV46         20000206.844  120p  Had.VSOLJ
HadV46         20000305.810  106p  Had.VSOLJ

Observer's code:
  Had: K. Haseda (Aichi, Japan)
       Instruments: 10cm F4.0 twin patrol camera +T-Max400(120)

Relayed from Katsumi Haseda <haseda@mxs.mesh.ne.jp>

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