The luminous erupting dwarf nova CV 1 in the dense globular cluster M15

Michael M. Shara, Sasha Hinkley, David R. Zurek, Christian Knigge, Howard E. Bond

Research output: Contribution to journalArticlepeer-review

7 Scopus citations


Despite decades-old predictions of the expected presence of dozens of cataclysmic variables in the cores of globular clusters, the number of irrefutable, outbursting candidates is still barely a handful. Using multiwavelength, multiepoch Hubble Space Telescope images, we have produced outburst and quiescence light curves for the recently discovered large-amplitude variable CV 1 in the core of the post-core-collapse globular cluster M15. The light curves and blue colors show that the object is a bona fide dwarf nova, with absolute magnitude at maximum light rivaling that of the most luminous known dwarf novae.

Original languageEnglish (US)
Pages (from-to)2847-2853
Number of pages7
JournalAstronomical Journal
Issue number6
StatePublished - Dec 2004

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science


Dive into the research topics of 'The luminous erupting dwarf nova CV 1 in the dense globular cluster M15'. Together they form a unique fingerprint.

Cite this