CG Draconis, a particularly active dwarf nova

Simple item page
dc.creatorShears, Jeremy
dc.creatorPickard, Roger
dc.creatorPoyner, Gary
dc.date2006-08-03
dc.date.accessioned2026-07-07T07:19:17Z
dc.date.available2026-07-07T07:19:17Z
dc.descriptionThe dwarf nova CG Dra was intensively monitored during 2005 as part of the Variable Star Sections Recurrent Objects Programme and seven outbursts were detected. These observations were combined with others from the BAA and AAVSO databases which confirmed that the star shows frequent outbursts with a period of around 11 days. Two types of outburst have been detected. Short outbursts lasting about 4 days and long outbursts lasting about 8 days.
dc.descriptionAccepted for publication in Journal of the British Astronomical Association 3 pages, 3 figures, 2 tables
dc.identifierhttps://arxiv.org/abs/astro-ph/0608081
dc.identifierhttp://arxiv.org/abs/astro-ph/0608081
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/114570
dc.subjectAstrophysics
dc.titleCG Draconis, a particularly active dwarf nova
dc.typetext

Files

Collections

arXiv