2MASS J05162881+2607387 is a Double-Lined Eclipsing Low-Mass Binary

Details 2MASS J05162881+2607387 is a Double-Lined Eclipsing Low-Mass Binary 2MASS J05162881+2607387 is a Double-Lined Eclipsing Low-Mass Binary

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..680....1b&link_type=abstract

The Astronomer's Telegram, #680

Astronomy and Astrophysics

Astronomy

Optical, Binaries, Variables

Scientific paper

The star known as 2MASS J05162881+2607387 (J0516) was discovered to be an eclipsing binary by Schuh et al. (2003, A&A, 410, 649). Assuming that the orbital period is the same as the eclipse period (1.29395 days), Schuh et al. suggested that J0516 consists of a K7V star and a brown dwarf. Schuh et al. also considered the possibility that the orbital period of J0156 was twice the eclipse period .

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