Predicting the properties of binary stellar systems: The evolution of accreting protobinary systems

Monthly Notices of the Royal Astronomical Society

Volumn 314, Issue 1, 2000, Pages 33-53

  Bate, Matthew R ^a,b  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

Accretion, accretion discs; Binaries: general; Circumstellar matter; Stars: formation; Stars: low mass, brown dwarfs; Stars: luminosity function, mass function

Indexed keywords

EXTRASOLAR PLANETS; FORECASTING; ORBITS; STARS;

ACCRETION: ACCRETION DISKS; BINARIES:GENERAL; CIRCUMSTELLAR MATTERS; MASS FUNCTIONS; MOLECULAR CLOUDS; PROPERTY; STAR: LUMINOSITY FUNCTION, MASS FUNCTION; STARS FORMATION; STARS: LOW-MASS BROWN DWARFS; STARS: LUMINOSITY FUNCTION;

SEPARATION;

EID: 0001999029     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03333.x     Document Type: Article

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