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J/AcA/62/33 OGLE II detached red giant eclipsing binary twins (Nataf+, 2012)
Detached red giant eclipsing binary twins: Rosetta stones to the Galactic Bulge. Nataf D.M., Gould A., Pinsonneault M.H. <Acta Astron., 62, 33-65 (2012)> =2012AcA....62...33N
ADC_Keywords: Binaries, eclipsing ; Stars, giant Keywords: Galaxy: bulge - Galaxy: stellar content - binaries: eclipsing Abstract: We identify 34 highly-probable detached, red giant eclipsing binary pairs among 315 candidates in Devor's catalog of ∼10000 OGLE-II eclipsing binaries. We estimate that there should be at least 200 such systems in OGLE-III. We show that spectroscopic measurements of the metallicities and radial-velocity-derived masses of these systems would independently constrain both the age-metallicity and helium-metallicity relations of the Galactic bulge, potentially breaking the age-helium degeneracy that currently limits our ability to characterize the bulge stellar population. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table12.dat 96 282 OGLE-II identification, coordinates, apparent magnitudes, relative radii and periods for the gold and silver sample RG eclipsing binary pairs identified (tables 1 & 2 of the paper)
See also: J/ApJ/628/411 : Identification & analysis of eclipsing binaries (Devor+, 2005) Byte-by-byte Description of file: table12.dat
Bytes Format Units Label Explanations
1 A1 --- S [GS] Gold or Silver sample 3- 4 I2 --- Field Field number (1) 6- 9 I4 --- LCNum Star number within the field (1) 11- 12 I2 h RAh Right ascension (J2000) 14- 15 I2 min RAm Right ascension (J2000) 17- 21 F5.2 s RAs Right ascension (J2000) 23 A1 --- DE- Declination sign (J2000) 24- 25 I2 deg DEd Declination (J2000) 27- 28 I2 arcmin DEm Declination (J2000) 30- 33 F4.1 arcsec DEs Declination (J2000) 35- 39 F5.3 mag V-I OGLE V-I colour index (2) 41- 46 F6.3 mag Imag OGLE I magnitude (2) 48- 52 F5.3 --- R1/a Radius of small star, in units of semimajor axis 54- 58 F5.3 --- R2/a Radius of large star, in units of semimajor axis 60- 68 F9.6 d Per Orbital period 70- 74 F5.3 --- Ecc Orbital eccentricity 76- 85 F10.2 d T0 Epoch for the secondary eclipse (when the secondary is behind the primary) 87- 90 F4.2 d t1 Transit time 92- 96 F5.3 --- sini Sine of inclination
Note (1): The star IDs used here are those from the catalog of Devor (2005, Cat. J/ApJ/628/411), <OGLEII DIA BUL-SCNN NNNN> in Simbad. More detailed properties can be found in the catalog of Devor (2005, Cat. J/ApJ/628/411). Note (2): The original photometry for these sources can be found on the OGLE-II archive (Udalski et al. 1997AcA....47..319U; Szymanski et al. 2005AcA....55...43S).
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 10-May-2012
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