Radius and mass of a transiting M dwarf near the hydrogen-burning limit - OGLE-TR-123

• Type: Article in International Scientific Journal
• Date: 2006

Authors

Pont, F (Author) Other; Moutou, C (Author) Other; Bouchy, F (Author) Other; Behrend, R (Author) Other; Mayor, M (Author) Other; Udry, S (Author) Other; Queloz, D (Author) Other; N.C. Santos (Author) Other; Melo, C (Author) Other

Journal

Title: Astronomy and Astrophysics

Vol. 447

Pages: 1035-1039

ISSN: 0004-6361

Publisher: EDP Sciences

Indexing

ISI Web of Knowledge - 44 Citations

Scopus - 42 Citations

Other information

Authenticus ID: P-004-MVK

DOI: 10.1051/0004-6361:20053692

Abstract (EN): The system OGLE-TR-123, detected by the OGLE planetary transit survey in Carina, was shown by subsequent spectroscopic follow-up to be an eclipsing binary with a very low mass companion (M-2 similar to 0.07 M.). Neither the light curve nor the radial velocity data were sufficient to constrain the parameters more precisely and to exclude alternative explanations in terms of a triple system. In this paper, new HARPS radial velocity data and a precise photometric monitoring of the transit with VLT/FORS2 are presented, resulting in an improved mass and radius determination for OGLE-TR-123b and the rejection of alternative scenarios. We find M-2 = 0.085 +/- 0.011 M. and R-2 = 0.133 +/- 0.009 R. for the transiting companion, confirming its nature as a small M dwarf near the hydrogen-burning limit. Its mass-radius relation corresponds to expectations for a relatively young object. The primary is an F dwarf that does not rotate synchronously with the orbital motion. Asynchronous rotation is unexpected in such a close binary (P = 1.8 days) but could be explained by the small mass of the secondary, the young age for the system, and the absence of convective envelope in the primary. OGLE-TR-123b is one of only two known objects below 0.1 M. with directly determined radii, after a similar object was characterised around OGLE-TR-122. The characterisation of OGLE-TR-123 provides another example of the type of system that can closely mimic planetary transits and contaminate transit surveys.

Language: English

Type (Professor's evaluation): Scientific

No. of pages: 5