The Star Formation Rate of Supersonic Magnetohydrodynamic Turbulence
Research output: Contribution to journal › Journal article › Research › peer-review
Standard
The Star Formation Rate of Supersonic Magnetohydrodynamic Turbulence. / Padoan, Paolo; Nordlund, Åke.
In: Astrophysical Journal, Vol. 730, No. 1, 20.03.2011, p. 40.Research output: Contribution to journal › Journal article › Research › peer-review
Harvard
Padoan, P & Nordlund, Å 2011, 'The Star Formation Rate of Supersonic Magnetohydrodynamic Turbulence', Astrophysical Journal, vol. 730, no. 1, pp. 40. https://doi.org/10.1088/0004-637X/730/1/40
APA
Padoan, P., & Nordlund, Å. (2011). The Star Formation Rate of Supersonic Magnetohydrodynamic Turbulence. Astrophysical Journal, 730(1), 40. https://doi.org/10.1088/0004-637X/730/1/40
Vancouver
Padoan P, Nordlund Å. The Star Formation Rate of Supersonic Magnetohydrodynamic Turbulence. Astrophysical Journal. 2011 Mar 20;730(1):40. https://doi.org/10.1088/0004-637X/730/1/40
Author
Bibtex
@article{8fdb0c6e120c464fb7db92693260eb30,
title = "The Star Formation Rate of Supersonic Magnetohydrodynamic Turbulence",
author = "Paolo Padoan and {\AA}ke Nordlund",
year = "2011",
month = mar,
day = "20",
doi = "10.1088/0004-637X/730/1/40",
language = "English",
volume = "730",
pages = "40",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "1",
}
RIS
TY - JOUR
T1 - The Star Formation Rate of Supersonic Magnetohydrodynamic Turbulence
AU - Padoan, Paolo
AU - Nordlund, Åke
PY - 2011/3/20
Y1 - 2011/3/20
U2 - 10.1088/0004-637X/730/1/40
DO - 10.1088/0004-637X/730/1/40
M3 - Journal article
VL - 730
SP - 40
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 1
ER -
ID: 37771985