Eclipse timings of the low-mass X-ray binary EXO 0748-676: Statistical arguments against orbital period changes

Abstract

view Abstract Citations (16) References (49) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Eclipse Timings of the Low-Mass X-Ray Binary EXO 0748-676: Statistical Arguments against Orbital Period Changes Hertz, Paul ; Wood, Kent S. ; Cominsky, Lynn Abstract EXO 0748-676, an eclipsing low-mass X-ray binary, is one of only about four or five low-mass X-ray binaries for which orbital period evolution has been reported. We observed a single eclipse egress with ROSAT . The time of this egress is consistent with the apparent increase in Porb previously reported on the basis of EXOSAT and Ginga observations. Standard analysis, in which O-C (observed minus calculated) timing residuals are examined for deviations from a constant period, implicitly assume that the only uncertainty in each residual is measurement error and that these errors are independent. We argue that the variable eclipse durations and profiles observed in EXO 0748-676 imply that there is an additional source of uncertainty in timing measurements, that this uncertainty is intrinsic to the binary system, and that it is correlated from observation to observation with a variance which increases as a function of the number of binary cycles between observations. This intrinsic variability gives rise to spurious trends in O-C residuals which are misinterpreted as changes in the orbital period. We describe several statistics tests which can be used to test for the presence of intrinsic variability. We apply those statistical tests which are suitable to the EXO 0748-676 observations. The apparent changes in the orbital period of EXO 0748-676 can be completely accounted for by intrinsic variability with an rms variability of approximately 0.35 s per orbital cycle. The variability appears to be correlated from cycle-to-cycle on timescales of less than 1 yr. We suggest that the intrinsic variability is related to slow changes in either the source's X-ray luminosity or the structure of the companion star's atmosphere. We note that several other X-ray binaries and cataclysmic variables have previously reported orbital period changes which may also be due to intrinsic variability rather than orbital period evolution. Publication: The Astrophysical Journal Pub Date: January 1995 DOI: 10.1086/175082 Bibcode: 1995ApJ...438..385H Keywords: Eclipsing Binary Stars; Statistical Analysis; Stellar Mass; Time Measurement; Variability; X Ray Binaries; Companion Stars; Error Analysis; Orbital Mechanics; Rosat Mission; Astrophysics; STARS: BINARIES: ECLIPSING; STARS: INDIVIDUAL ALPHANUMERIC: EXO 0748-676; X-RAYS: STARS full text sources ADS | data products SIMBAD (8) HEASARC (1)