Different modes of star formation: gravitational collapse of magnetically subcritical cloud
Author:
Affiliation:
1. Department of Earth and Planetary Sciences, Faculty of Sciences, Kyushu University, Fukuoka 812-8581, Japan
2. Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8511, Japan
Funder
JSPS
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/473/3/3080/21688260/stx2589.pdf
Reference86 articles.
1. ALMA OBSERVATIONS OF THE TRANSITION FROM INFALL MOTION TO KEPLERIAN ROTATION AROUND THE LATE-PHASE PROTOSTAR TMC-1A
2. Outflows and Jets from Collapsing Magnetized Cloud Cores
3. Magnetic braking, ambipolar diffusion, and the formation of cloud cores and protostars. 1: Axisymmetric solutions
4. Magnetic Braking, Ambipolar Diffusion, and the Formation of Cloud Cores and Protostars. II. A Parameter Study
5. Magnetic Braking, Ambipolar Diffusion, and the Formation of Cloud Cores and Protostars. III. Effect of the Initial Mass-to-Flux Ratio
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