The initial mass function of the Orion nebula cluster across the H-burning limit

Astrophysical Journal

Volumn 748, Issue 1, 2012, Pages

  Da Rio, N ^a   Robberto, M ^b   Hillenbrand, L A ^c   Henning, T ^d   Stassun, K G ^e,f,g  

^a EUROPEAN SPACE AGENCY   (Netherlands)

^b STScI   (United States)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^e VANDERBILT UNIVERSITY   (United States)

^f FISK UNIVERSITY   (United States)

^g MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

brown dwarfs; Hertzsprung Russell and C M diagrams; open clusters and associations: individual (Orion); stars: formation; stars: luminosity function, mass function; stars: pre main sequence

Indexed keywords

EID: 84858029064     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/748/1/14     Document Type: Article

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