Collapse of Magnetized Singular Isothermal Toroids. II. Rotation and Magnetic Braking
暂无分享,去创建一个
[1] Kohji Tomisaka,et al. Collapse-Driven Outflow in Star-Forming Molecular Cores , 1998 .
[2] M. Norman,et al. ZEUS-2D: A radiation magnetohydrodynamics code for astrophysical flows in two space dimensions. I - The hydrodynamic algorithms and tests. II - The magnetohydrodynamic algorithms and tests , 1992 .
[3] J. Fiege,et al. Prolate Cores in Filamentary Molecular Clouds , 1999, astro-ph/9909356.
[4] S. Desch,et al. The Magnetic Decoupling Stage of Star Formation , 2001 .
[5] Tomisaka. The Evolution of the Angular Momentum Distribution during Star Formation. , 1999, The Astrophysical journal.
[6] Enhancement of Ambipolar Diffusion Rates through Field Fluctuations , 2002, astro-ph/0201131.
[7] A. Toomre,et al. On the gravitational stability of a disk of stars , 1964 .
[8] Bruce T. Draine,et al. in Protostars and Planets II , 1985 .
[9] E. Ostriker,et al. Low-Mass Star Formation: Theory , 1999 .
[10] P. Caselli,et al. L1544: A Starless Dense Core with Extended Inward Motions , 1998 .
[11] A. Goodman,et al. Dense cores in dark clouds. VI - Shapes , 1991 .
[12] F. Shu,et al. Collapse of Magnetized Molecular Cloud Cores. II. Numerical Results , 1993 .
[13] C. Lada,et al. Spectral evolution of young stellar objects , 1986 .
[14] A. Toomre. Some flattened isothermal models of galaxies , 1982 .
[15] C. Lada,et al. Book-Review - the Physics of Star Formation and Early Stellar Evolution , 1991 .
[16] T. Mouschovias. Single-Stage Fragmentation and a Modern Theory of Star Formation , 1991 .
[17] S. Miyama,et al. Analytic Solutions for Equilibrium of Rotating Isothermal Clouds -- One-Parameter Family of Axisymmetric and Conformal Configurations-- , 1982 .
[18] F. Shu,et al. Molecular cloud cores and bimodal star formation , 1989 .
[19] A. Boss,et al. Protostars and Planets VI , 2000 .
[20] F. Shu,et al. Collapse of magnetized molecular cloud cores. I: Semianalytical solution , 1993 .
[21] E. Zweibel,et al. Current Sheet Formation in the Interstellar Medium , 1997 .
[22] D. Ward-Thompson,et al. First Observations of the Magnetic Field Geometry in Prestellar Cores , 2000 .
[23] J. Najita,et al. X-Ray Ionization of Protoplanetary Disks , 1997 .
[24] R. Larson. The physics of star formation , 2003, astro-ph/0306595.
[25] U. Virginia,et al. Binary and Multiple Star Formation in Magnetic Clouds: Bar Growth and Fragmentation , 2003, astro-ph/0305317.
[26] S. Basu,et al. Magnetic braking, ambipolar diffusion, and the formation of cloud cores and protostars. I. Axisymmetric solutions , 1994 .
[27] Richard M. Crutcher,et al. Magnetic Fields in Molecular Clouds: Observations Confront Theory , 1998 .
[28] G. Laughlin,et al. Singular Isothermal Disks. II. Nonaxisymmetric Bifurcations and Equilibria , 2000, astro-ph/0012242.
[29] R. Nishi,et al. Magnetic flux loss from interstellar clouds with various grain-size distributions , 1991 .
[30] Alyssa A. Goodman,et al. Measurement of Magnetic Field Strength in the Dark Cloud Barnard 1 , 1989 .
[31] Telemachos Ch. Mouschovias,et al. in The Origin of Stars and Planetary Systems , 1999 .
[32] M. Reid,et al. OH masers and the Galactic magnetic field , 1990 .
[33] F. Shu,et al. Relativistic Singular Isothermal Toroids , 2003, astro-ph/0302474.
[34] V. Ferraro. The non-uniform rotation of the Sun and its magnetic field , 1937 .
[35] Y. Fukui. Molecular clouds and star formation , 2005 .
[36] B. Wilson. Magnetic Fields in Star-forming Molecular Clouds. V. Submillimeter Polarization of the Barnard 1 Dark Cloud , 2002, astro-ph/0205328.
[37] R. Crutcher,et al. OH Zeeman Measurement of the Magnetic Field in the L1544 Core , 2000 .
[38] Frank H. Shu,et al. Magnetized Singular Isothermal Toroids , 1996 .
[39] K. Tomisaka. Collapse of Rotating Magnetized Molecular Cloud Cores and Mass Outflows , 2001, astro-ph/0105527.
[40] M. Claussen,et al. High-resolution observations of ionized gas in central 3 parsecs of the Galaxy: possible evidence for infall , 1983, Nature.
[41] Zhi-Yun Li,et al. Self-Similar Collapse of an Isopedic Isothermal Disk , 1997 .
[42] F. Shu,et al. Heating and Ionization of X-Winds , 2001, astro-ph/0110539.
[43] Peter Goldreich,et al. I. Gravitational Stability of Uniformly Rotating Disks , 1965 .
[44] F. Adams,et al. Star Formation in Molecular Clouds: Observation and Theory , 1987 .
[45] P. Andre',et al. Molecular line study of the very young protostar IRAM 04191 in Taurus: Infall, rotation, and outflow , 2002, astro-ph/0207287.
[46] Andrea Richichi,et al. A lunar occultation and direct imaging survey of multiplicity in the Ophiuchus and Taurus star-forming regions , 1995 .
[47] STRUCTURE AND EVOLUTION OF MAGNETICALLY SUPPORTED MOLECULAR CLOUDS : EVIDENCE FOR AMBIPOLAR DIFFUSION IN THE BARNARD 1 CLOUD , 1994 .
[48] Charles J. Lada,et al. The Origin of Stars and Planetary Systems , 1999 .
[49] Alyssa A. Goodman,et al. Dense cores in dark clouds. VIII - Velocity gradients , 1993 .
[50] Telemachos Ch. Mouschovias,et al. Magnetic Fields and Star Formation: A Theory Reaching Adulthood , 1999 .
[51] Zhi-Yun Li,et al. Hydromagnetic Accretion Shocks around Low-Mass Protostars , 1996 .
[52] F. Motte,et al. Discovery of an Extremely Young Accreting Protostar in Taurus , 1999 .
[53] F. Shu,et al. Relativistic Self-similar Disks , 2001, astro-ph/0111344.
[54] G. Blake,et al. High-Resolution 4.7 micron Keck/NIRSPEC Spectra of Protostars. I. Ices and Infalling Gas in the Disk of L1489 IRS , 2001, astro-ph/0112163.