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Ground‐ and space‐based study of two globular cluster cataclysmic variables: M22 CV1 and M5 V101

dc.contributor.authorHourihane, A. P.en_US
dc.contributor.authorCallanan, P. J.en_US
dc.contributor.authorCool, A. M.en_US
dc.contributor.authorReynolds, Mark T.en_US
dc.date.accessioned2011-11-10T15:36:36Z
dc.date.available2012-07-12T17:42:24Zen_US
dc.date.issued2011-06-11en_US
dc.identifier.citationHourihane, A. P.; Callanan, P. J.; Cool, A. M.; Reynolds, M. T. (2011). "Ground‐ and space‐based study of two globular cluster cataclysmic variables: M22 CV1 and M5 V101." Monthly Notices of the Royal Astronomical Society 414(1). <http://hdl.handle.net/2027.42/87033>en_US
dc.identifier.issn0035-8711en_US
dc.identifier.issn1365-2966en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87033
dc.description.abstractAs a class of compact binaries with large binding energy, cataclysmic variables (CVs) formed through close encounters play an important role in the dynamical evolution of globular clusters. As part of a systematic search for CVs undergoing dwarf nova (DN) eruptions in globular clusters, our 2004 monitoring programme of M22 detected an outburst of the DN candidate CV1 during May. We implement the isis image subtraction routine to obtain a light curve for an outburst of CV1. We present the outburst light curve as well as Hubble Space Telescope /Wide‐Field Planetary Camera 2 (WFPC2) photometry in the V , U and near‐ultraviolet ( nUV ) bands and a Chandra /Advanced CCD Imaging Spectrometer (ACIS) spectrum of the object. Our results confirm the DN nature of the outburst and the CV status of the object. We also present the results of a ground‐based study of another globular cluster CV, M5 V101 – including quiescent medium‐resolution William Herschel Telescope (WHT)/Intermediate dispersion Spectrograph and Imaging System (ISIS) spectroscopy in the B and R bands, displaying prominent Balmer and He  i emission, and R ‐band photometry.en_US
dc.publisherBlackwell Publishing Ltden_US
dc.publisherWiley Periodicals, Inc.en_US
dc.subject.otherTechniques: Photometricen_US
dc.subject.otherStars: Dwarf Novaeen_US
dc.subject.otherX‐Rays: Binariesen_US
dc.titleGround‐ and space‐based study of two globular cluster cataclysmic variables: M22 CV1 and M5 V101en_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationotherDepartment of Physics, University College Cork, Cork, Irelanden_US
dc.contributor.affiliationotherDepartment of Physics and Astronomy, San Francisco State University, 1600 Holloway Avenue, San Francisco, CA 94132, USAen_US
dc.identifier.pmid21643840en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/87033/1/j.1365-2966.2011.18364.x.pdf
dc.identifier.doi10.1111/j.1365-2966.2011.18364.xen_US
dc.identifier.sourceMonthly Notices of the Royal Astronomical Societyen_US
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