CDROM/AJ/V109/P0359 H235 in NGC 752 (Milone+ 1995) ================================================================================ Observations and Analysis of the Contact Binary H235 in the Open Cluster NGC 752 E. F. Milone, C. R. Stagg, B. A. Sugars, J. R. McVean, S. J. Schiller, J. Kallrath & D. H. Bradstreet <1995, AJ, 109, 359> =1995AJ....109..359M ================================================================================ Abstract: The short-period variable star Heinemann 235 in the open cluster NGC 752 has been identified as a contact binary with a variable period of about 0.4118 d. BVRI light curves and radial velocity curves have been obtained and analyzed with enhanced versions of the Wilson-Devinney light curve program. We find that the system is best modeled as an A-type W UMa system, with a contact parameter of 0.21 +/- 0.11. The masses of the components are found to be 1.18 +/- 0.17 and 0.24 +/- 0.04 Msun, with bolometric magnitudes of 3.60 +/- 0.10 and 5.21 +/- 0.13, for the hotter (6500 K, assumed) and cooler (6421 K) components, respectively, with Delta T = 79 +/- 25 K. The distance to the binary is established at 381 +/- 17 pc. H235 becomes one of a relatively small number of open-cluster contact systems with detailed light curve analysis for which an age may be estimated. If it is coeval with the cluster, and with the detached eclipsing and double-lined spectroscopic binary H219 (DS And), H235 is ~1.8 Gyr old, and may provide a fiducial point for the evolution of contact systems. There is, however, evidence for dynamical evolution of the cluster and the likelihood of weak interactions over the age of the binary precludes the determination of its initial state with certainty. File Summary: -------------------------------------------------------------------------------- File Name Lrecl Records Explanations -------------------------------------------------------------------------------- table3.dat 78 867 Photoelectric light curve data -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1-10 F10.4 d HJD Heliocentric Julian Date - 2400000 11-18 F8.4 --- Ph1 *Phase of minima from ephemeris 1 19-26 F8.4 --- Ph3 *Phase of minima from ephemeris 3 27-33 F7.3 mag dV Differential V magnitude 34-40 F7.3 mag dB Differential B magnitude 41-47 F7.3 mag dR Differential R magnitude 48-54 F7.3 mag dI Differential I magnitude 55-62 F8.3 mag d(B-V) Differential (B-V) color 63-70 F8.3 mag d(V-R) Differential (V-R) color 71-78 F8.3 mag d(V-I) Differential (V-I) color -------------------------------------------------------------------------------- Notes for file: table3.dat -------------------------------------------------------------------------------- Ph1: Phase of minima calculated using ephemeris (1) from printed paper: E0 = 2 447 815.338(3), P = 0.411 83(12)d Ph3: Phase of minima calculated using ephemeris (3) from printed paper: E0 = 2 446 785.8660(23), P = 0.411 775 0(10)d -------------------------------------------------------------------------------- ================================================================================ (End) Lee Brotzman [ADS] 29-Apr-1995