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Michael J. Cai, Ph.D. - Publications

Affiliations: 
2002 University of California, Berkeley, Berkeley, CA, United States 
Area:
Astronomy and Astrophysics
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9 high-probability publications. We are testing a new system for linking publications to authors. You can help! If you notice any inaccuracies, please sign in and mark papers as correct or incorrect matches. If you identify any major omissions or other inaccuracies in the publication list, please let us know.

Year Citation  Score
2011 Adams FC, Cai MJ, Galli D, Lizano S, Shu FH. Magnetic interactions in pre-main-sequence binaries Astrophysical Journal. 743. DOI: 10.1088/0004-637X/743/2/175  0.653
2010 Cai MJ, Taam RE. The equilibrium structure of prolate magnetized molecular cores Astrophysical Journal Letters. 709: L79-L82. DOI: 10.1088/2041-8205/709/1/L79  0.423
2010 Lizano S, Galli D, Cai MJ, Adams FC. Stability of magnetized disks and implications for planet formation Astrophysical Journal. 724: 1561-1570. DOI: 10.1088/0004-637X/724/2/1561  0.709
2010 Galli D, Shu FH, Lizano S, Cai MJ. The role of magnetic fields in the protostellar accretion phase Aip Conference Proceedings. 1242: 231-242. DOI: 10.1063/1.3460129  0.694
2009 Adams FC, Cai MJ, Lizano S. Migration of extrasolar planets: Effects from x-wind accretion disks Astrophysical Journal. 702: L181-L186. DOI: 10.1088/0004-637X/702/2/L182  0.636
2008 Shu FH, Lizano S, Galli D, Cai MJ, Mohanty S. The challenge of sub-Keplerian rotation for disk winds Astrophysical Journal. 682: L121-L124. DOI: 10.1086/591028  0.69
2008 Cai MJ, Shang H, Lin HH, Shu FH. X-winds in action Astrophysical Journal. 672: 489-503. DOI: 10.1086/523788  0.657
2007 Shu FH, Galli D, Lizano S, Cai MJ. Magnetization, accretion, and outflows in young stellar objects Proceedings of the International Astronomical Union. 3: 249-264. DOI: 10.1017/S1743921307009611  0.705
2004 Cai MJ, Shu FH. Non-axisymmetric modes in relativistic singular isothermal disks Progress of Theoretical Physics Supplement. 155: 317-318. DOI: 10.1143/Ptps.155.317  0.568
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