What causes the low binary frequency in the Orion Nebula Cluster?
Document title: What causes the low binary frequency in the Orion Nebula Cluster?
Journal: Revista mexicana de astronomía y astrofísica. Serie de conferencias
Database: PERIÓDICA
System number: 000228004
ISSN: 1405-2059
Authors: 1
Institutions: 1MPI fur Astronomie, Heidelberg, Baden-Wurttemburg. Alemania
Year:
Season: Ago
Volumen: 21
Pages: 104-108
Country: México
Language: Inglés
Document type: Conferencia o discurso
Approach: Descriptivo, aplicado
Disciplines: Física y astronomía
Keyword: Astronomía,
Física,
Astrofísica,
Estrellas dobles,
Nebulosa de Orión,
Formación de estrellas,
Estrellas jóvenes
Keyword: Physics and astronomy,
Astronomy,
Physics,
Astrophysics,
Double stars,
Orion Nebula,
Stars formation,
Young stars
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