The First DIRECT Distance Determination to a Detached Eclipsing Binary in M33
Author(s) -
A. Z. Bonanos,
K. Z. Stanek,
R. P. Kudritzki,
Lucas M. Macri,
Dimitar Sasselov,
J. Kałużny,
P. B. Stetson,
D. Bersier,
Fabio Bresolin,
T. Matheson,
B. J. Mochejska,
N. Przybilla,
Á. Szentgyörgyi,
J. Tonry,
Guillermo Torres
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/508140
Subject(s) - photometry (optics) , distance modulus , physics , astrophysics , binary number , stars , spectroscopy , light curve , galaxy , astronomy , mathematics , arithmetic
We present the first direct distance determination to a detached eclipsingbinary in M33, which was found by the DIRECT Project. Located in the OB 66association at coordinates (alpha, delta)=(01:33:46.17,+30:44:39.9) forJ2000.0, it was one of the most suitable detached eclipsing binaries found byDIRECT for distance determination, given its apparent magnitude and orbitalperiod. We obtained follow-up BV time series photometry, JHKs photometry andoptical spectroscopy from which we determined the parameters of the system. Itcontains two O7 main sequence stars with masses of 33.4+/-3.5 Mo and 30.0+/-3.3Mo and radii of 12.3+/-0.4 Ro and 8.8+/-0.3 Ro, respectively. We derivetemperatures of 37000+/-1500 K and 35600+/-1500 K. Using BVRJHKs photometry forthe flux calibration, we obtain a distance modulus of 24.92+/-0.12 mag(964+/-54 kpc), which is ~0.3 mag longer than the Key Project distance to M33.We discuss the implications of our result and the importance of establishingM33 as an independent rung on the cosmological distance ladder.Comment: 36 pages, 12 figures, accepted for publication in Ap
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