Telemachos C. Mouschovias - Publications

Affiliations: 
1977- University of Illinois, Urbana-Champaign, Urbana-Champaign, IL 
Area:
Astronomy and Astrophysics
Website:
https://physics.illinois.edu/people/directory/profile/tchm

43 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
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  0.719
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  0.748
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  0.774
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  0.806
2005 Tassis K, Mouschovias TC. Magnetically controlled spasmodic accretion during star formation. II. Results Astrophysical Journal. 618: 783-794. DOI: 10.1086/424480  0.784
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  0.78
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  0.616
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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