V 877 ARA

SU UMa-type dwarf novae.

2002-06-09 SSO Observations

V877 Ara: new SU UMa-type dwarf nova!

,

    On 9 june Roland Santallo Southern Stars Observatory, Tahiti French Polynesia
conduct time-series photometry of V877 Ara (NSV08383)
The data show fully developed superhumps (amplitude 0.25-0.30 mag),
establishing that V877 Ara is a new member of SU UMa-type dwarf novae.
Although exact period determination is still difficult on single-night
data, the system has a relatively long (around 0.08 d) superhump period.
Observers are strongly urged to continue observation as long as possible
(prefreably more than two superhump cycles per night) in order to precisely
determine the superhump period.

    !

*******
V877 Ara image and position

From Taichi Kato VSnet Team


    This object seems to be correpond to

USNO0225.27372547 171653.966 -653251.46 (2000.0) 20.3 21.6

    which is different from previous identidications.  More detailed
identification awaits Yamaoka-san's astrometry (Vsnet Team).  The quiescent counterpart
seems to be much fainter than was previously thought.  This is consistent
with the superhump detection.

    Anyway, observers should refer to the above image before observing,
since the position has a large offset from the GCVS/NSV/Downes catalogs.
Further obseravtions are very strongly requested!


 

 

S.S.O Light Curve

Run TIME SERIE 2002-06-09

The Superhumps are Full developed

Light curve from Vsnet on S.S.O Images

Comments from Taichi Kato VSnet team

Roland Santallo (Southern Stars Observatory, Tahiti French Polynesia) just reported time-series photometry of V877 Ara (NSV08383) taken on June 9. The data show fully developed superhumps (amplitude 0.25-0.30 mag), establishing that V877 Ara is a new member of SU UMa-type dwarf novae. Although exact period determination is still difficult on single-night data, the system has a relatively long (around 0.08 d) superhump period. Observers are strongly urged to continue observation as long as possible (prefreably more than two superhump cycles per night) in order to precisely determine the superhump period.

Congratulations to Roland Santallo on this breath-taking success!

 

Astrophysic Abstract Astro-ph 0210674