Open AccessPhotometric study of the variable star population in the globular cluster NGC 6397
Author(s) -
Kaluzny J.,
Thompson I. B.,
Krzeminski W.,
SchwarzenbergCzerny A.
Publication year - 2006
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2005.09734.x
Subject(s) - physics , globular cluster , astrophysics , millisecond pulsar , astronomy , cataclysmic variable star , dwarf nova , variable star , light curve , photometry (optics) , stars , pulsar , white dwarf
We present the results of a photometric survey for variable stars in the central region of the nearby globular cluster NGC 6397. Time‐series photometry was obtained for 30 variable objects. The sample includes 12 new objects, of which six show periodic light curves and two are eclipsing binaries of unknown period. Six variables possess certain and three possess likely X‐ray counterparts detected with the Chandra observatory. Among them, four are cataclysmic variables and one is a foreground eclipsing binary. The cataclysmic variable CV2 exhibited a likely dwarf nova type outburst in 2003 May. The cataclysmic variable CV3 was observed at 18.5 < V < 20.0 during five observing runs, but went into a low state in 2003 May when it reached V > 22 . We have found that the light curve of the optical companion to the millisecond pulsar PSR J1740−5340 exhibits noticeable changes of its amplitude on a time‐scale of a few months. A shallow eclipse with Δ V = 0.03 mag was detected in one of the cluster turn‐off stars suggesting the presence of a large planet or brown dwarf in orbit.