Virtual Journal of Nuclear Astrophysics
Edited by
Honey Arora
, Michigan State University and
Fry Fang
, University of Notre Dame
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Radiation-Hydrodynamic Simulations of Massive Star Formation with Protostellar Outflows
Virtual Journal - Volume 9, Issue 14 - article #6
Andrew J. Cunningham
,
Richard I. Klein
,
Mark R. Krumholz
,
Christopher F. McKee
arXiv.org - Astrophysics - Volume: 2011, Issue: 8 Apr
arXiv:1104.1218
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pdf
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other
]
Metallicity and the Universality of the IMF
Virtual Journal - Volume 9, Issue 6 - article #2
Andrew T. Myers
,
Mark R. Krumholz
,
Richard I. Klein
,
Christopher F. McKee
arXiv.org - Astrophysics - Volume: 2011, Issue: 11 Feb
arXiv:1102.2023
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pdf
,
other
]
The Formation of Massive Star Systems by Accretion
Virtual Journal - Volume 7, Issue 6 - article #18
Mark R. Krumholz
,
Richard I. Klein
,
Christopher F. McKee
,
Stella S. R. Offner
,
and
Andrew J. Cunningham<br />
,
Science - Volume: 323, Issue: 5915
Published online 15 January 2009 [DOI: 10.1126/science.1165857] (in
Science
Express Reports)
Numerical simulations show that instabilities can channel gas into growing massive stars despite their high radiation pressure.
Abstract »
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The formation of stars by gravitational collapse rather than competitive accretion
Virtual Journal - Volume 3, Issue 46 - article #44
Mark R. Krumholz
,
Christopher F. McKee
and
Richard I. Klein
Nature – Vol. 438, Issue 7066 – November 2005
First paragraph
,
Full Text
,
PDF (111K)
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Supplementary information
Stars Form By Gravitational Collapse, Not Competitive Accretion
Virtual Journal - Volume 3, Issue 42 - article #20
Mark R. Krumholz
(1),
Christopher F. McKee
(2 and 3),
Richard I. Klein
(3 and 4)
((1) Department of Astrophysical Sciences, Princeton University,
(2) Department of Physics, University of California, Berkeley,
(3) Department of Astronomy, University of California, Berkeley,
(4) Lawrence Livermore National Laboratory)
ArXiv - Astrophysics – October 2005
astro-ph/0510412 [
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