Improving PARSEC models for very low mass stars

Monthly Notices of the Royal Astronomical Society

Volumn 444, Issue 3, 2014, Pages 2525-2543

  Chen, Yang ^a,b   Girardi, Léo ^c   Bressan, Alessandro ^a   Marigo, Paola ^d   Barbieri, Mauro ^d   Kong, Xu ^b,e  

^a SISSA   (Italy)

^b UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

^c INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^d UNIVERSITY OF PADOVA   (Italy)

^e INSTITUTE OF GEOLOGY AND GEOPHYSICS   (China)

Author keywords

Hertzsprung Russell and colour magnitude diagrams; Stars: Evolution; Stars: Low mass

Indexed keywords

ASTROPHYSICS; COLOR; INFRARED DEVICES; PHOTOMETRY;

COLOR-MAGNITUDE DIAGRAMS; COLOUR-MAGNITUDE DIAGRAMS; HERTZSPRUNG-RUSSELL; HERTZSPRUNG-RUSSELL AND COLOR-MAGNITUDE DIAGRAM; OPTICAL-; STAR: EVOLUTION; STARS: LOW MASS; STELLAR EVOLUTIONS; TRIESTE; VERY-LOW-MASS STARS;

CALIBRATION;

EID: 84914670160     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stu1605     Document Type: Article

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