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Astrophysics > Solar and Stellar Astrophysics

arXiv:1306.5908 (astro-ph)
[Submitted on 25 Jun 2013]

Title:Variability survey in the CoRoT SRa01 field: Implications of eclipsing binary distribution on cluster formation in NGC 2264

Authors:P. Klagyivik, Sz. Csizmadia, T. Pasternacki, T. Fruth, A. Erikson, J. Cabrera, R. Chini, P. Eigmüller, P. Kabath, S. Kirste, R. Lemke, M. Murphy, H. Rauer, R. Titz-Weider
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Abstract:Time-series photometry of the CoRoT field SRa01 was carried out with the Berlin Exoplanet Search Telescope II (BEST II) in 2008/2009. A total of 1,161 variable stars were detected, of which 241 were previously known and 920 are newly found. Several new, variable young stellar objects have been discovered. The study of the spatial distribution of eclipsing binaries revealed the higher relative frequency of Algols toward the center of the young open cluster NGC 2264. In general Algol frequency obeys an isotropic distribution of their angular momentum vectors, except inside the cluster, where a specific orientation of the inclinations is the case. We suggest that we see the orbital plane of the binaries almost edge-on.
Comments: 18 pages, 8 figures, accepted for publication in ApJ
Subjects: Solar and Stellar Astrophysics (astro-ph.SR)
Cite as: arXiv:1306.5908 [astro-ph.SR]
  (or arXiv:1306.5908v1 [astro-ph.SR] for this version)
  https://doi.org/10.48550/arXiv.1306.5908
Related DOI: https://doi.org/10.1088/0004-637X/773/1/54

Submission history

From: Péter Klagyivik [view email]
[v1] Tue, 25 Jun 2013 10:23:42 UTC (9,156 KB)
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