The stellar initial mass function from turbulent fragmentation
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Standard
The stellar initial mass function from turbulent fragmentation. / Nordlund, Åke; Padoan, Paolo.
I: Astrophysical Journal, Nr. 576, 2002, s. 870-879.Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt
Harvard
Nordlund, Å & Padoan, P 2002, 'The stellar initial mass function from turbulent fragmentation', Astrophysical Journal, nr. 576, s. 870-879.
APA
Nordlund, Å., & Padoan, P. (2002). The stellar initial mass function from turbulent fragmentation. Astrophysical Journal, (576), 870-879.
Vancouver
Nordlund Å, Padoan P. The stellar initial mass function from turbulent fragmentation. Astrophysical Journal. 2002;(576):870-879.
Author
Bibtex
@article{57c3550074c511dbbee902004c4f4f50,
title = "The stellar initial mass function from turbulent fragmentation",
author = "{\AA}ke Nordlund and Paolo Padoan",
year = "2002",
language = "English",
pages = "870--879",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "576",
}
RIS
TY - JOUR
T1 - The stellar initial mass function from turbulent fragmentation
AU - Nordlund, Åke
AU - Padoan, Paolo
PY - 2002
Y1 - 2002
M3 - Journal article
SP - 870
EP - 879
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 576
ER -
ID: 130000