Discovery of a new SU UMa-type dwarf nova V344 Lyrae

Details Discovery of a new SU UMa-type dwarf nova V344 Lyrae Discovery of a new SU UMa-type dwarf nova V344 Lyrae

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasj...45l..67k&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan, vol. 45, no. 6, p. L67-L71

Astronomy and Astrophysics

Astronomy

14

Accretion Disks, Cataclysmic Variables, Dwarf Novae, Main Sequence Stars, Astronomical Photometry, Charge Coupled Devices, Stellar Magnitude

Scientific paper

A faint dwarf nova, V344 Lyrae, was observed for five nights in its long outburst during May-June, 1993. V-band Charge Coupled Device (CCD) photometry revealed superhumps with a period of 0.09145 (+/- 0.00002) d and an amplitude of 0.3 mag. This finding confirms V344 Lyrae as being a new member of SU UMa-type dwarf novae and places it as the second longest orbital-period dwarf nova below the period gap. The cycle lengths of the normal outbursts and superoutbursts have been estimated to be 16 +/- 3 d and 240 d, respectively.

Affiliated with

Also associated with

No associations

Rating

Discovery of a new SU UMa-type dwarf nova V344 Lyrae 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 new SU UMa-type dwarf nova V344 Lyrae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Discovery of a new SU UMa-type dwarf nova V344 Lyrae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1301135