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A runaway collision in a young star cluster as the origin of the brightest supernova

Author
PORTEGIES ZWART, Simon F1 2 ; VAN DEN HEUVEL, Edward P. J1 3
[1] Stronomical Institute 'Anton Pannekoek', University of Amsterdam, Kruislaan 403, Netherlands
[2] Institute for Computer Science, University of Amsterdam, Kruislaan 403, Netherlands
[3] Kavli Institute for Theoretical Physics, University of California Santa Barbara, California 93 106-4030, United States
Source

Nature (London). 2007, Vol 450, Num 7168, pp 388-389, 2 p ; ref : 30 ref

CODEN
NATUAS
ISSN
0028-0836
Scientific domain
Multidisciplinary
Publisher
Nature Publishing, London
Publication country
United Kingdom
Document type
Article
Language
English
Keyword (fr)
Amas jeune Amas stellaire Etoile en cavale Etoile massive Fréquence collision Supernova extragalactique
Keyword (en)
Young cluster Star clusters Runaway stars Massive stars Collision frequency Extragalactic supernova
Keyword (es)
Cúmulo joven Frecuencia colisión Supernova extragaláctica
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D10 Stellar dynamics and kinematics

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D20 Stellar clusters and associations / 001E03D20D Open clusters in the milky way

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D20 Stellar clusters and associations / 001E03D20G Globular clusters in the milky way

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
19221902

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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