Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994pasj...46l.199k&link_type=abstract
PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 46, no. 6, p. L199-L202
Astronomy and Astrophysics
Astronomy
7
Cataclysmic Variables, Dwarf Novae, Stellar Magnitude, Astrometry, Astronomical Photometry
Scientific paper
A faint dwarf nova, KV And, was observed for two nights during its long outburst in 1993 November. V-band CCD photometry revealed superhumps with a period of 0.07520 (+/- 0.00003) d or its alias 0.07427 (+/- 0.00003) d, and an amplitude of 0.28 mag. This discovery confirms KV And as being a new member of SU UMa-type dwarf novae, and makes it as a good candidate for being a TOAD (Tremendous Amplitude Dwarf Nova).
Kato Taichi
Kunjaya Chatief
Okyudo Masami
Takahashi Atsushi
No associations
LandOfFree
Discovery of a large-amplitude SU UMa-type dwarf nova, KV Andromedae does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Discovery of a large-amplitude SU UMa-type dwarf nova, KV Andromedae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Discovery of a large-amplitude SU UMa-type dwarf nova, KV Andromedae will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1414297