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[vsnet-obs 8785] oddleiv.skilbrei@statkart.no, dahle@galileo.IFA.Hawaii.Edu, henninho@astro.uio.no, bgranslo@astro.uio.no



Norwegian Astronomical Society - Variable Star Section

Visual observations by observers of NAS.VSS (Report 1997h-060):

Object       YYMMDD(UT)   Mag   Obs. Instrum.   Notes
AQLV         971201.71    7.7   GRL  L70;24x
BOOV         971201.73    8.6   GRL  L70;24x
CASrho       971201.73    4.8   GRL  B10x50
CETomicron   971201.76    6.0   GRL  B10x50     Brightening
CRBR         971201.73    6.0   GRL  B10x50
CRBS         971201.73    7.6   GRL  L70;24x
CYGAF        971201.72    7.2   GRL  L70;24x
CYGCH        971201.72    9.2   GRL  L70;24x
CYGchi       971201.72    7.7   GRL  L70;24x    Fading
DELEU        971201.71    6.3   GRL  L70;24x
DELU         971201.71    7.0   GRL  L70;24x
DRAAG        971201.72    9.9   GRL  L70;24x
DRAAH        971201.72    8.4   GRL  L70;24x
DRARY        971201.72    7.2   GRL  L70;24x
DRATX        971201.72    7.6   GRL  L70;24x
HERX         971201.72    6.8   GRL  L70;24x
OPHX         971201.73    7.4   GRL  L70;24x
PEGAG        971201.71    8.8   GRL  L70;24x
PERX         971201.73    6.3   GRL  B10x50
SCTR         971201.71    5.3   GRL  L70;24x
UMIV         971201.72    8.1   GRL  L70;24x

Note: Mira (Omicron Ceti) is brightening rapidly, currently by
  nearly 0.25 mag. per day.

Observers:
GRL = Bjorn H. Granslo (Blindern, Oslo, Norway). Instruments: 70-mm
  refractor (L70), 10x50 binoculars (B10x50). Partly cloudy. AAVSO
  sequences were used. Venus was observed for a few minutes before
  it set. Green flashes were visible in the telescope and Venus
  appeared red and dimmed by 6.5-8.0 mag. (slowly fluctuating) due
  to the strong extinction. Its apparent brightness was compared
  with stars near zenith. When Venus set at 16h56m UT its true
  altitude was -0.6 deg., i.e. below the astronomical horizon.

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