Spiral-arm instability – II. Magnetic destabilization
Author:
Affiliation:
1. Kavli Institute for the Physics and Mathematics of the Universe (WPI), UTIAS, The University of Tokyo, Chiba 277-8583, Japan
2. Department of Physics, School of Science, The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
Funder
World Premier International Research Center Initiative
Ministry of Education, Culture, Sports, Science and Technology
Japan Science and Technology Agency
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/485/3/3024/28079589/stz584.pdf
Reference103 articles.
1. HIGH-RESOLUTION STUDY OF THE CLUSTER COMPLEXES IN A LENSED SPIRAL AT REDSHIFT 1.5: CONSTRAINTS ON THE BULGE FORMATION AND DISK EVOLUTION
2. Local interstellar gasdynamical stability and substructure in spiral arms
3. DYNAMO – II. Coupled stellar and ionized-gas kinematics in two low-redshift clumpy discs
4. Structure formation in gas-rich galactic discs with finite thickness: from discs to rings
5. Galactic Dynamics
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