Luminosity discrepancy in the equal-mass, pre-main-sequence eclipsing binary par 1802: Non-coevality or tidal heating?

Astrophysical Journal

Volumn 745, Issue 1, 2012, Pages

  Gómez Maqueo Chew, Yilen ^a,b   Stassun, Keivan G ^a,c,d   Prša, Andrej ^e,f   Stempels, Eric ^g   Hebb, Leslie ^a   Barnes, Rory ^h   Heller, René ⁱ   Mathieu, Robert D ^j  

^a VANDERBILT UNIVERSITY   (United States)

^b QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^c FISK UNIVERSITY   (United States)

^d MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^e VILLANOVA UNIVERSITY   (United States)

^f UNIVERSITY OF LJUBLJANA   (Slovenia)

^g UPPSALA UNIVERSITY   (Sweden)

^h UNIVERSITY OF WASHINGTON   (United States)

ⁱ ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^j UNIVERSITY OF WISCONSIN MADISON   (United States)

more..

Author keywords

binaries: eclipsing; stars: fundamental parameters; stars: individual (Parenago 1802); stars: low mass; stars: pre main sequence

Indexed keywords

EID: 84855765264     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/745/1/58     Document Type: Article

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