Massive binaries as the source of abundance anomalies in globular clusters

Astronomy and Astrophysics

Volumn 507, Issue 1, 2009, Pages

  De Mink, S E ^a   Pols, O R ^a   Langer, N ^a,b   Izzard, R G ^c  

^a UTRECHT UNIVERSITY   (Netherlands)

^b UNIVERSITY OF BONN   (Germany)

^c UNIVERSITÉ LIBRE DE BRUXELLES   (Belgium)

Author keywords

Galaxy: globular clusters: general; ISM: general; Stars: abundances; Stars: binaries: close

Indexed keywords

AGB STARS; ALTERNATIVE SOURCE; ASYMPTOTIC GIANT BRANCH STARS; BREAK-UP; GALAXY: GLOBULAR CLUSTERS: GENERAL; GLOBULAR CLUSTERS; INITIAL MASS; INTERSTELLAR MEDIUMS; ISM: GENERAL; LOW VELOCITIES; LOW-MASS STARS; LOW-VELOCITY; M STARS; MASS STARS; MASSIVE STARS; POTENTIAL WELLS; PRIMARY STARS; SECOND GENERATION; TIDAL INTERACTIONS;

GALAXIES; HELIUM; MATERIALS; ROTATION; SODIUM; SPIN DYNAMICS; SUPERCONDUCTING WIRE;

STARS;

EID: 70449687183     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913205     Document Type: Article

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