The Magnetic Fields of Classical T Tauri Stars
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[1] L. Hartmann,et al. Emission-Line Diagnostics of T Tauri Magnetospheric Accretion. II. Improved Model Tests and Insights into Accretion Physics , 2001 .
[2] R. Pudritz,et al. The spin of accreting stars: dependence on magnetic coupling to the disc , 2004, astro-ph/0409701.
[3] Alan T. Tokunaga,et al. CSHELL: a high spectral resolution 1-5-μm cryogenic echelle spectrograph for the IRTF , 1993, Defense, Security, and Sensing.
[4] H. Spruit,et al. Convective instability of thin flux tubes , 1979 .
[5] J. Valenti,et al. Spectroscopic Properties of Cool Stars (SPOCS). I. 1040 F, G, and K Dwarfs from Keck, Lick, and AAT Planet Search Programs , 2005 .
[6] William H. Press,et al. Numerical recipes , 1990 .
[7] L. Wallace,et al. Medium-Resolution Spectra of Normal Stars in the K Band , 1997 .
[8] S. Fabrika,et al. Possible variability of the magnetic field of T Tau , 2004 .
[9] S. Matt,et al. Accretion-powered Stellar Winds as a Solution to the Stellar Angular Momentum Problem , 2005, astro-ph/0510060.
[10] L. Hartmann,et al. Magnetospheric Accretion Models for the Hydrogen Emission Lines of T Tauri Stars , 1998 .
[11] E. Feigelson,et al. High-Energy Processes in Young Stellar Objects , 1999 .
[12] G. Basri,et al. The Spectral Variability of the Classical T Tauri Star DR Tauri , 2001 .
[13] R. Kurucz,et al. Convective Intensification of Magnetic Flux Tubes in Stellar Photospheres , 2002, astro-ph/0201026.
[14] I. Roxburgh,et al. On the generation of the large-scale and turbulent magnetic fields in solar-type stars , 1993 .
[15] S. Saar. Recent measurements of stellar magnetic fields , 1996 .
[16] S. Lamzin,et al. Analysis of magnetic field measurements for T Tau , 2005 .
[17] J. Valenti,et al. Detection of Strong Magnetic Fields on M Dwarfs , 1995 .
[18] L. Wallace,et al. An atlas of a dark sunspot umbral spectrum from 1970 to 8640 cm(-1) (1.16 to 5.1 [microns]) , 1992 .
[19] J. Valenti,et al. Spectral Synthesis of TiO Lines , 1998 .
[20] S. Saar. Magnetic Fields on Solar-Like Stars: The First Decade , 1990 .
[21] M. Camenzind. Magnetized Disk-Winds and the Origin of Bipolar Outflows. , 1990 .
[22] K. Shibata,et al. X-Ray Flares and Mass Outflows Driven by Magnetic Interaction between a Protostar and Its Surrounding Disk , 1996, astro-ph/9606157.
[23] G. Marcy,et al. Limits on the Magnetic Flux of a Pre-Main Sequence Star , 1992 .
[24] J. Valenti,et al. T Tauri stars in blue , 1993 .
[25] J. Valenti,et al. An IUE Atlas of Pre-Main-Sequence Stars. II. Far-Ultraviolet Accretion Diagnostics in T Tauri Stars , 2000 .
[26] J. Linsky,et al. The photospheric magnetic field of the dM3.5e flare star AD Leonis , 1985 .
[27] R. Winglee,et al. Jets from Accreting Magnetic Young Stellar Objects. I. Comparison of Observations and High-Resolution Simulation Results , 1999 .
[28] G. Wallerstein,et al. Cool stars, stellar systems, and the sun : Sixth Cambridge Workshop , 1990 .
[29] A. Boss,et al. Protostars and Planets VI , 2000 .
[30] Does Disk Locking Solve the Stellar Angular Momentum Problem , 2004, astro-ph/0403635.
[31] New Tests of Magnetospheric Accretion in T Tauri Stars , 2002, astro-ph/0205190.
[32] D. F. Gray. Observations of spectral line asymmetries and convective velocities in F, G and K stars. , 1982 .
[33] Testing the reality of strong magnetic fields on T Tauri stars: The naked T Tauri star Hubble 4 , 2004, astro-ph/0409268.
[34] J. Stone,et al. Magnetohydrodynamic Simulations of Stellar Magnetosphere-Accretion Disk Interaction , 1997 .
[35] K. Stassun,et al. X-Ray Properties of Pre-Main-Sequence Stars in the Orion Nebula Cluster with Known Rotation Periods , 2004, astro-ph/0403159.
[36] A. Koenigl. Disk accretion onto magnetic T Tauri stars , 1991 .
[37] S. Sciortino,et al. Time evolution of X-ray coronal activity in PMS stars; a possible relation with the evolution of accretion disks , 2003, astro-ph/0302329.
[38] L. Hillenbrand,et al. Disk Accretion in the 10 Myr Old T Tauri Stars TW Hydrae and Hen 3-600A , 2000, The Astrophysical journal.
[39] C. Tinney. The Bottom of the Main Sequence — And Beyond , 1995 .
[40] R. Tayler. Magnetic activity in pre-main-sequence stars , 1987 .
[41] Donald N. B. Hall,et al. Design for a 1--5-um cryogenic echelle spectrograph for the NASA IRTF , 1990, Astronomical Telescopes and Instrumentation.
[42] X-RAYS IN THE ORION NEBULA CLUSTER: CONSTRAINTS ON THE ORIGINS OF MAGNETIC ACTIVITY IN PRE-MAIN-SEQUENCE STARS , 2002, astro-ph/0211049.
[43] J. Ferreira,et al. Reconnection X‐winds: spin‐down of low‐mass protostars , 2000 .
[44] P. Ghosh,et al. Accretion by rotating magnetic neutron stars. II. Radial and vertical structure of the transition zone in disk accretion. , 1979 .
[45] G. Basri,et al. Hamilton echelle spectra of young stars. I: Optical veiling , 1990 .
[46] P. Hauschildt. M (sub)Dwarf Model Atmospheres: The Next Generation , 1995 .
[47] O. Regev,et al. Photometric Observations of YY Orionis: New Insight Into the Accretion Process , 1996 .
[48] B. Krauskopf,et al. Proc of SPIE , 2003 .
[49] J. Valenti,et al. Infrared Zeeman Analysis of epsilon Eridani , 1995 .
[50] Keivan G. Stassun,et al. The Rotation Period Distribution of Pre-Main-Sequence Stars in and around the Orion Nebula , 1999 .
[51] E. Ostriker,et al. Magnetocentrifugally Driven Flows from Young Stars and Disks. IV. The Accretion Funnel and Dead Zone , 1995 .
[52] B. Durney,et al. On the angular momentum loss of late-type stars , 1977 .
[53] J. Valenti,et al. The Large-Scale Axisymmetric Magnetic Topology of a Very-Low-Mass Fully Convective Star , 2006, Science.
[54] T Tauri stellar magnetic fields: He i measurements , 2005, astro-ph/0501445.
[55] L. Hartmann,et al. Calcium II infrared triplet line models in classical T Tauri stars , 2006, 0712.2971.
[56] M. F. Skrutskie,et al. Near-Infrared Photometric Monitoring of Young Stellar Objects , 1996 .
[57] A. V. Koldoba,et al. THREE-DIMENSIONAL SIMULATIONS OF DISK ACCRETION TO AN INCLINED DIPOLE. II. HOT SPOTS AND VARIABILITY , 2004, astro-ph/0404496.
[58] L. Hartmann,et al. Additional measurements of pre-main-sequence stellar rotation , 1989 .
[59] S. Saar. Improved Methods for the Measurement and Analysis of Stellar Magnetic Fields , 1988 .
[60] P. Demarque,et al. The theoretical calculation of the Rossby number and the `non-local' convective overturn time for pre-main sequence and early post-main sequence stars , 1995, astro-ph/9507096.
[61] J. Stenflo. Solar photosphere: Structure, convection and magnetic fields , 1989 .
[62] L. Hartmann,et al. Rotational and radial velocities of T Tauri stars , 1986 .
[63] J. Valenti,et al. Measuring the Magnetic Field of the Classical T Tauri Star TW Hydrae , 2005, astro-ph/0509549.
[64] J. Gosling,et al. The relationship between large-scale solar magnetic field evolution and coronal mass ejections , 1998 .
[65] G. G. Valyavin,et al. Possible detection of a magnetic field in T Tauri , 2003, astro-ph/0302026.
[66] N. Schulz,et al. Evidence for Accretion: High-Resolution X-Ray Spectroscopy of the Classical T Tauri Star TW Hydrae , 2001, astro-ph/0111049.
[67] E. Feigelson,et al. The Origin of T Tauri X-Ray Emission: New Insights from the Chandra Orion Ultradeep Project , 2005, astro-ph/0506526.
[68] J. Valenti,et al. Spectropolarimetry of Magnetospheric Accretion on the Classical T Tauri Star BP Tauri , 1998 .
[69] A. Harris,et al. On the simultaneous optical and near-infrared variability of pre-main sequence stars , 2002 .
[70] J. Valenti,et al. New Infrared Veiling Measurements and Constraints on Accretion Disk Models for Classical T Tauri Stars , 2001 .
[71] K. Wood,et al. X-ray emission from T Tauri stars , 2006, astro-ph/0601213.
[72] K. Keil,et al. Protostars and Planets V , 2007 .
[73] S. Saar. New Infrared Measurements of Magnetic Fields on Cool Stars , 1994 .
[74] H. L. Johnson,et al. Astronomical Measurements in the Infrared , 1966 .
[75] Robert Winglee,et al. Time-dependent Accretion by Magnetic Young Stellar Objects as a Launching Mechanism for Stellar Jets , 1997 .
[76] G. Basri,et al. The Line Profile Variability of SU Aurigae , 1995 .
[77] N. Calvet,et al. The Structure and Emission of the Accretion Shock in T Tauri Stars , 1998 .
[78] P. Hartigan,et al. Disk Accretion and Mass Loss from Young Stars , 1995 .
[79] Austin,et al. Observational Constraints on the Formation and Evolution of Binary Stars , 2001, astro-ph/0103098.
[80] Jr. Robinson. Magnetic field measurements on stellar sources - A new method , 1980 .
[81] E. Recillas,et al. The Hot SPOT in DR Tauri , 1994 .
[82] P. Hartigan,et al. Spectroscopic evidence for magnetospheric accretion in classical T Tauri stars , 1994 .
[83] A. Pevtsov,et al. The Relationship Between X-Ray Radiance and Magnetic Flux , 2003 .
[84] S. Solanki,et al. Three dimensional structure of a regular sunspot from the inversion of IR Stokes profiles , 2003 .
[85] C. Bertout,et al. Accretion Disks around T Tauri Stars , 1988 .
[86] J. Valenti,et al. Observations of Magnetic Fields on T Tauri Stars , 2004 .
[87] S. Baliunas,et al. Rotation, convection, and magnetic activity in lower main-sequence stars , 1984 .
[88] W. Dobler,et al. Magnetic Field Generation in Fully Convective Rotating Spheres , 2006 .
[89] Christopher D. Koresko,et al. Measuring the Magnetic Field on the Classical T Tauri Star BP Tauri , 1999 .
[90] L. Hartmann,et al. Disk Accretion Rates for T Tauri Stars , 1998 .
[91] Mass accretion on to T Tauri stars , 2006, astro-ph/0606682.
[92] D. Padgett. Atmospheric Parameters and Iron Abundances of Low-Mass Pre-Main-Sequence Stars in Nearby Star Formation Regions , 1996 .
[93] D. Moss. The survival of fossil magnetic fields during pre-main sequence evolution , 2003 .
[94] S. Edwards,et al. Helium Emission from Classical T Tauri Stars: Dual Origin in Magnetospheric Infall and Hot Wind , 2001 .
[95] Large-scale alpha^2-dynamo in low-mass stars and brown dwarfs , 2005, astro-ph/0510075.
[96] S. Sciortino,et al. Einstein Observations of T Tauri Stars in Taurus-Auriga. I. Properties of X-Ray Emission , 1995 .