The luminosity function of the globular cluster NGC 6752 with the Hubble Space Telescope: Evidence of mass segregation

Monthly Notices of the Royal Astronomical Society

Volumn 286, Issue 4, 1997, Pages 1012-1022

  Ferraro, F R ^a   Carretta, E ^a   Bragaglia, A ^a   Renzini, A ^b,c   Ortolani, S ^d  

^a INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c UNIVERSITY OF BOLOGNA   (Italy)

^d UNIVERSITY OF PADOVA   (Italy)

Author keywords

Galaxy: stellar content; Globular clusters: individual: NGC 6752; Hertzsprung Russell (HR) diagram; Stars: fundamental parameters; Stars: low mass, brown dwarfs

Indexed keywords

SPACE TELESCOPES; STARS;

GALAXY:STELLAR CONTENT; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS: INDIVIDUAL: NGC 6752; GROUND-BASED OBSERVATIONS; HERTZSPRUNG-RUSSELL DIAGRAMS; LUMINOSITY FUNCTIONS; MASS SEGREGATION; STARS: LOW-MASS BROWN DWARFS; STARS:FUNDAMENTAL PARAMETERS;

LUMINANCE;

EID: 0040915831     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/286.4.1012     Document Type: Article

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