An international team of astronomers has performed photometric observations of a binary system known as CXOGBS J175553.2-281633. Results of the study indicate that the object is a cataclysmic variable system. The finding is reported in a paper published September 18 on arXiv.org.
Cataclysmic variables are binary star systems consisting of a white dwarf primary that is accreting matter from a normal star companion. They irregularly increase in brightness by a large factor, then drop back down to a quiescent state. These binaries have been found in many environments, such as the center of the Milky Way galaxy, the solar neighborhood, and within open and globular clusters.
CXOGBS J175553.2-281633, or CX137, was initially detected as an X-ray source by the Galactic Bulge Survey (GBS). In 2012, the optical counterpart to CX137 identiﬁed and classiﬁed as an eclipsing binary with a spotted donor star and an orbital period of approximately 10.345 hours.
Now, a group of astronomers led by Sebastian Gomez of the Harvard-Smithsonian Center for Astrophysics (CfA) in Cambridge, Massachusetts, present the results of a long-term monitoring campaign of CX137 as part of the Optical Gravitational Lensing Experiment (OGLE) project. The observations, conducted with the 1.3-meter Warsaw telescope at Las Campanas Observatory, provide more insights into the nature of this source.
“We have modeled seven years of optical photometry of the binary star CX137,” the researchers wrote in the paper.
The observational campaign detected long-term variations of CX137 from year to year. According to the authors of the study, such behavior can be explained with either an accretion disk of changing shape or luminosity, or a spotted secondary star. The orbital period of the system was estimated to be 10.34488 hours,