The mass-radius relationship for very low mass stars: Four new discoveries from the HATSouth Survey

Monthly Notices of the Royal Astronomical Society

Volumn 437, Issue 3, 2014, Pages 2831-2844

  Zhou, G ^a   Bayliss, D ^a   Hartman, J D ^b,c   Bakos, G A ^b,c   Penev, K ^b,c   Csubry, Z ^b,c   Tan, T G ^d   Jordan A ^e   Mancini, L ^f   Rabus, M ^e   Brahm, R ^e   Espinoza, N ^e   Mohler Fischer, M ^f   Ciceri, S ^f   Suc, V ^e   Csak B ^f   Henning, T ^f   Schmidt, B ^a  

^a AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^b PRINCETON UNIVERSITY   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d Perth Exoplanet Survey Telescope   (Australia)

^e PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^f MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Binaries; Eclipsing stars; Low mass.

Indexed keywords

STARS;

BINARY; BINARY SYSTEMS; ECLIPSING-STARS; GLOBAL ANALYSIS; HIGH RESOLUTION; ISOCHRONES; LOW-MASS; LOW-MASS.; PRIMARY STARS; VERY-LOW-MASS STARS;

SURVEYS;

EID: 84891369910     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stt2100     Document Type: Article

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