Year |
Citation |
Score |
2015 |
Tritsis A, Panopoulou GV, Mouschovias TC, Tassis K, Pavlidou V. Magnetic field-gas density relation and observational implications revisited Monthly Notices of the Royal Astronomical Society. 451: 4384-4396. DOI: 10.1093/Mnras/Stv1133 |
0.773 |
|
2011 |
Mouschovias TC, Ciolek GE, Morton SA. Hydromagnetic waves in weakly-ionized media - I. Basic theory, and application to interstellar molecular clouds Monthly Notices of the Royal Astronomical Society. 415: 1751-1782. DOI: 10.1111/J.1365-2966.2011.18817.X |
0.451 |
|
2010 |
Mouschovias TC, Tassis K. Self-consistent analysis of OH-Zeeman observations: Too much noise about noise Monthly Notices of the Royal Astronomical Society. 409: 801-807. DOI: 10.1111/J.1365-2966.2010.17345.X |
0.678 |
|
2010 |
Tassis K, Christie DA, Urban A, Pineda JL, Mouschovias TC, Yorke HW, Martel H. Do lognormal column-density distributions in molecular clouds imply supersonic turbulence? Monthly Notices of the Royal Astronomical Society. 408: 1089-1094. DOI: 10.1111/J.1365-2966.2010.17181.X |
0.678 |
|
2010 |
Kunz MW, Mouschovias TC. The non-isothermal stage of magnetic star formation - II. Results Monthly Notices of the Royal Astronomical Society. 408: 322-341. DOI: 10.1111/J.1365-2966.2010.17110.X |
0.806 |
|
2009 |
Mouschovias TC, Tassis K. Testing molecular-cloud fragm0065ntation theories: Self-consistent analysis of OH Zeeman observations Monthly Notices of the Royal Astronomical Society: Letters. 400: L15-L19. DOI: 10.1111/J.1745-3933.2009.00752.X |
0.714 |
|
2009 |
Kunz MW, Mouschovias TC. The initial core mass function due to ambipolar diffusion in molecular clouds Monthly Notices of the Royal Astronomical Society: Letters. 399. DOI: 10.1111/J.1745-3933.2009.00731.X |
0.717 |
|
2009 |
Mouschovias TC, Kunz MW, Christie DA. Formation of interstellar clouds: Parker instability with phase transitions Monthly Notices of the Royal Astronomical Society. 397: 14-23. DOI: 10.1111/J.1365-2966.2009.14472.X |
0.777 |
|
2009 |
Kunz MW, Mouschovias TC. ERRATUM: “THE NONISOTHERMAL STAGE OF MAGNETIC STAR FORMATION. I. FORMULATION OF THE PROBLEM AND METHOD OF SOLUTION” (2009, APJ, 693, 1895) The Astrophysical Journal. 696: 2290-2290. DOI: 10.1088/0004-637X/696/2/2290 |
0.747 |
|
2009 |
Kunz MW, Mouschovias TC. The nonisothermal stage of magnetic star formation. I. Formulation of the problem and method of solution Astrophysical Journal. 693: 1895-1911. DOI: 10.1088/0004-637X/693/2/1895 |
0.773 |
|
2008 |
Chiang HF, Looney LW, Tassis K, Mundy LG, Mouschovias TC. Constraining the earliest circumstellar disks and their envelopes Astrophysical Journal. 680: 474-482. DOI: 10.1086/588036 |
0.683 |
|
2007 |
Tassis K, Mouschovias TC. Protostar formation in magnetic molecular clouds beyond ion detachment. III. A parameter study Astrophysical Journal. 660: 402-417. DOI: 10.1086/512762 |
0.789 |
|
2007 |
Tassis K, Mouschovias TC. Protostar formation in magnetic molecular clouds beyond ion detachment. II. Typical axisymmetric solution Astrophysical Journal. 660: 388-401. DOI: 10.1086/512761 |
0.781 |
|
2007 |
Tassis K, Mouschovias TC. Protostar formation in magnetic molecular clouds beyond ion detachment. I. Formulation of the problem and method of solution Astrophysical Journal. 660: 370-387. DOI: 10.1086/512760 |
0.784 |
|
2006 |
Mouschovias TC, Tassis K, Kunz MW. Observational constraints on the ages of molecular clouds and the star formation timescale: Ambipolar-diffusion-controlled or turbulence-induced star formation? Astrophysical Journal. 646: 1043-1049. DOI: 10.1086/500125 |
0.805 |
|
2005 |
Tassis K, Mouschovias TC. Magnetically controlled spasmodic accretion during star formation. II. Results Astrophysical Journal. 618: 783-794. DOI: 10.1086/424480 |
0.783 |
|
2005 |
Tassis K, Mouschovias TC. Magnetically controlled spasmodic accretion during star formation. I. Formulation of the problem and method of solution Astrophysical Journal. 618: 769-782. DOI: 10.1086/424479 |
0.779 |
|
2004 |
Tassis K, Mouschovias TC. Ambipolar-diffusion timescale, star formation timescale, and the ages of molecular clouds: Is there a discrepancy? Astrophysical Journal. 616: 283-287. DOI: 10.1086/424901 |
0.712 |
|
2004 |
Ciolek GE, Roberge WG, Mouschovias TC. Multifluid, magnetohydrodynamic shock waves with grain dynamics. II. Dust and the critical speed for C shocks Astrophysical Journal. 610: 781-800. DOI: 10.1086/421765 |
0.416 |
|
2001 |
Desch SJ, Mouschovias TC. The magnetic decoupling stage of star formation Astrophysical Journal. 550: 314-333. DOI: 10.1086/319703 |
0.629 |
|
1998 |
Ciolek GE, Mouschovias TC. Effect of ambipolar diffusion on ion abundances in contracting protostellar cores Astrophysical Journal. 504: 280-289. DOI: 10.1086/306074 |
0.435 |
|
1997 |
Basu S, Mouschovias TC, Paleologou EV. Dynamical effects of the parker instability in the interstellar medium Astrophysical Journal. 480. DOI: 10.1086/310620 |
0.615 |
|
1996 |
Ciolek GE, Mouschovias TC. Effect of ambipolar diffusion on dust-to-gas ratio in protostellar cores Astrophysical Journal. 468: 749-754. DOI: 10.1086/177730 |
0.516 |
|
1996 |
Basu S, Mouschovias TC, Paleologou EV. Evolution of the Parker instability: MHD flows, shock waves, and other consequences Astrophysical Letters and Communications. 34: 333-338. |
0.337 |
|
1995 |
Mouschovias TC, Psatis D. Hydromagnetic waves and the linewidth-size relation in interstellar molecular clouds Astrophysical Journal. 444. DOI: 10.1086/187871 |
0.436 |
|
1995 |
Ciolek GE, Mouschovias TC. Ambipolar diffusion, interstellar dust, and the formation of cloud cores and protostars. IV. Effect of ultraviolet ionization and magnetically controlled infall rate Astrophysical Journal. 454: 194-216. DOI: 10.1086/176477 |
0.564 |
|
1995 |
Basu S, Mouschovias TC. Magnetic braking, ambipolar diffusion, and the formation of cloud cores and protostars. III. Effect of the initial mass-to-flux ratio Astrophysical Journal. 453: 271-283. DOI: 10.1086/176387 |
0.736 |
|
1995 |
Basu S, Mouschovias TC. Magnetic braking, ambipolar diffusion, and the formation of cloud cores and protostars. II. a parameter study Astrophysical Journal. 452: 386-400. DOI: 10.1086/176310 |
0.77 |
|
1994 |
Basu S, Mouschovias TC. Magnetic braking, ambipolar diffusion, and the formation of cloud cores and protostars. I. Axisymmetric solutions Astrophysical Journal. 432: 720-741. DOI: 10.1086/174611 |
0.73 |
|
1994 |
Crutcher RM, Mouschovias TC, Troland TH, Ciolek GE. Structure and evolution of magnetically supported molecular clouds: Evidence for ambipolar diffusion in the Barnard 1 cloud Astrophysical Journal. 427: 839-847. DOI: 10.1086/174189 |
0.547 |
|
1994 |
Ciolek GE, Mouschovias TC. Ambipolar diffusion, interstellar dust, and the formation of cloud cores and protostars. III. Typical axisymmetric solutions Astrophysical Journal. 425: 142-160. DOI: 10.1086/173971 |
0.438 |
|
1994 |
Morton SA, Mouschovias TC, Ciolek GE. Ambipolar diffusion, interstellar dust, and the formation of cloud cores and protostars. II. Numerical method of solution Astrophysical Journal. 421: 561-569. DOI: 10.1086/173671 |
0.569 |
|
1993 |
Ciolek GE, Mouschovias TC. Ambipolar diffusion, interstellar dust, and the formation of cloud cores and protostars. I. Basic physics and formulation of the problem Astrophysical Journal. 418: 774-793. DOI: 10.1086/173435 |
0.421 |
|
1993 |
Fiedler RA, Mouschovias TC. Ambipolar diffusion and star formation: Formation and contraction of axisymmetric cloud cores. II. Results Astrophysical Journal. 415: 680-700. DOI: 10.1086/173193 |
0.539 |
|
1992 |
Fiedler RA, Mouschovias TC. Ambipolar diffusion and star formation: Formation and contraction of axisymmetric cloud cores. I. Formulation of the problem and method of solution Astrophysical Journal. 391: 199-219. DOI: 10.1086/171336 |
0.584 |
|
1992 |
Mouschovias TC, Morton SA. Ambipolar diffusion, cloud cores, and star formation: Two-dimensional, cylindrically symmetric contraction. III. A further parameter study and magnetically controlled accretion rate Astrophysical Journal. 390: 166-180. DOI: 10.1086/171268 |
0.647 |
|
1992 |
Mouschovias TC, Morton SA. Ambipolar diffusion, cloud cores, and star formation: Two-dimensional, cylindrically symmetric contraction, II. Results and a length scale for protostellar cores Astrophysical Journal. 390: 144-165. DOI: 10.1086/171267 |
0.571 |
|
1991 |
Mouschovias TC. Magnetic braking, ambipolar diffusion, cloud cores, and star formation: Natural length scales and protostellar masses Astrophysical Journal. 373: 169-186. DOI: 10.1086/170035 |
0.647 |
|
1991 |
Mouschovias TC, Morton SA. Ambipolar diffusion, cloud cores, and star formation: Two-dimensional, cylindrically symmetric contraction. I. The issues, formulation of the problem, and method of solution Astrophysical Journal. 371: 296-316. DOI: 10.1086/169893 |
0.61 |
|
1982 |
Mouschovias TC. Interstellar magnetic fields Advances in Space Research. 2: 71-80. DOI: 10.1016/0273-1177(82)90290-3 |
0.613 |
|
1980 |
Mouschovias TC, Paleologou EV. The angular momentum problem and magnetic braking during star formation: Exact solutions for an aligned and a perpendicular rotator The Moon and the Planets. 22: 31-45. DOI: 10.1007/BF00896865 |
0.548 |
|
1979 |
Mouschovias TC. Ambipolar diffusion in interstellar clouds : a new solution The Astrophysical Journal. 228: 475. DOI: 10.1086/156868 |
0.566 |
|
1974 |
Mouschovias TC. Static Equilibria of the Interstellar Gas in the Presence of Magnetic and Gravitational Fields: Large-Scale Condensations The Astrophysical Journal. 192: 37-50. DOI: 10.1086/153032 |
0.484 |
|
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