A two-step initial mass function: Consequences of clustered star formation for binary properties

Astronomy and Astrophysics

Volumn 371, Issue 3, 2001, Pages 952-962

  Durisen, R H ^a,b   Sterzik, M F ^c   Pickett, B K ^d,e  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b INDIANA UNIVERSITY   (United States)

^c EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^d VALPARAISO UNIVERSITY   (United States)

^e PURDUE UNIVERSITY CALUMET   (United States)

Author keywords

Methods: statistical; Stars: binaries: general; Stars: formation; Stars: pre main sequence

Indexed keywords

EID: 0035355396     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20010390     Document Type: Article

References (52)