T. Mouschovias

发表

Note on the collapse of magnetic interstellar clouds.

L. Spitzer, T. Mouschovias, 1976 .

The angular momentum problem and magnetic braking - an exact time-dependent solution

T. Mouschovias, E. Paleologou, 1979 .

The non-isothermal stage of magnetic star formation - II. Results

T. Mouschovias, M. Kunz, Matthew W. Kunz, 2010, 1003.2722.

Expansion and broadening of coronal loop transients: A theoretical explanation

A. Poland, T. Mouschovias, 1978 .

Magnetic braking, ambipolar diffusion, cloud cores, and star formation: Natural length scales and protostellar masses

T. Mouschovias, 1991 .

The initial core mass function due to ambipolar diffusion in molecular clouds

T. Mouschovias, M. Kunz, 2009, 0908.0102.

Magnetic braking, ambipolar diffusion, and the formation of cloud cores and protostars. III. Effect of the initial mass-to-flux ratio

S. Basu, T. Mouschovias, 1995 .

Testing Molecular-Cloud Fragmentation Theories: Self-Consistent Analysis of OH Zeeman Observations

K. Tassis, T. Mouschovias, 2009, 0909.2031.

Nonhomologous contraction and equilibria of self-gravitating, magnetic interstellar clouds embedded in an intercloud medium: star formation. II. Results.

T. Mouschovias, 1976 .

Hydromagnetic waves in weakly-ionized media – I. Basic theory, and application to interstellar molecular clouds

S. Morton, T. Mouschovias, G. Ciolek, 2011, 1103.6037.

The Role of Magnetic Fields in the Formation of Stars

T. Mouschovias, 1981 .

Cosmic Magnetism and the Basic Physics of the Early Stages of Star Formation

T. Mouschovias, 1991 .

Interstellar magnetic fields

T. Mouschovias, 1982 .

Fragmentation and Collapse in Magnetic Molecular Clouds: Natural Length Scales and Protostellar Masses

T. Mouschovias, 1990 .

Magnetic fields in molecular clouds: Regulators of star formation

T. Mouschovias, 1989 .

Star formation in magnetic interstellar clouds. I - Interplay between theory and observations. II - Basic theory

T. Mouschovias, 1987 .

Protostar Formation in Magnetic Molecular Clouds beyond Ion Detachment. II. Typical Axisymmetric Solution

K. Tassis, T. Mouschovias, 2007, astro-ph/0702037.

Ambipolar Diffusion, Interstellar Dust, and the Formation of Cloud Cores and Protostars. III. Typical Axisymmetric Solutions

T. Mouschovias, G. Ciolek, 1994 .

Ambipolar diffusion and star formation : formation and contraction of axisymmetric cloud cores. II: Results

T. Mouschovias, R. Fiedler, 1993 .

Protostar Formation in Magnetic Molecular Clouds beyond Ion Detachment. I. Formulation of the Problem and Method of Solution

K. Tassis, T. Mouschovias, 2007, astro-ph/0702036.

Protostar Formation in Magnetic Molecular Clouds beyond Ion Detachment. III. A Parameter Study

K. Tassis, T. Mouschovias, 2007, astro-ph/0702038.

Magnetic braking, ambipolar diffusion, and the formation of cloud cores and protostars. I. Axisymmetric solutions

S. Basu, T. Mouschovias, 1994 .

The magnetic flux problem and ambipolar diffusion during star formation: one-dimensional collapse. II: Results

T. Mouschovias, E. Paleologou, R. Fiedler, 1985 .

Ambipolar-Diffusion Timescale, Star Formation Timescale, and the Ages of Molecular Clouds: Is There a Discrepancy?

K. Tassis, T. Mouschovias, 2004, astro-ph/0409089.

Formation of interstellar clouds: Parker instability with phase transitions

D. Christie, T. Mouschovias, M. Kunz, 2009, 0901.0914.

The effect of ambipolar diffusion on magnetic braking of molecular cloud cores: an exact, time-dependent solution

T. Mouschovias, E. Paleologou, 1986 .

Ambipolar diffusion in interstellar clouds : a new solution

T. Mouschovias, 1979 .

Constraining the Earliest Circumstellar Disks and Their Envelopes

L. Mundy, K. Tassis, Hsin-Fang Chiang, 2008, 0803.1272.

Ambipolar diffusion and star formation: Formation and contraction of axisymmetric cloud cores. I. Formulation of the problem and method of solution

T. Mouschovias, R. Fiedler, 1992 .

Ambipolar diffusion, interstellar dust, and the formation of cloud cores and protostars. IV. Effect of ultraviolet ionization and magnetically controlled infall rate

T. Mouschovias, G. Ciolek, 1995 .

Magnetic Braking, Ambipolar Diffusion, and the Formation of Cloud Cores and Protostars. II. A Parameter Study

S. Basu, T. Mouschovias, 1995 .

Nonhomologous contraction and equilibria of self-gravitating, magnetic interstellar clouds embedded in an intercloud medium: Star formation. I Formulation of the problem and method of solution

T. Mouschovias, 1976 .

Ambipolar Diffusion, Interstellar Dust, and the Formation of Cloud Cores and Protostars. I. Basic Physics and Formulation of the Problem

T. Mouschovias, G. Ciolek, 1993 .

Self-consistent analysis of OH-Zeeman observations: too much noise about noise

K. Tassis, T. Mouschovias, 2010, 1007.3741.

Single-Stage Fragmentation and a Modern Theory of Star Formation

T. Mouschovias, 1991 .

A connection between the rate of rotation of interstellar clouds, magnetic fields, ambipolar diffusion, and the periods of binary stars

T. Mouschovias, 1977 .

Recent OH Zeeman Observations: Do they Really Contradict the Ambipolar-Diffusion Theory of Star Formation?

K. Tassis, T. Mouschovias, 2008, 0807.4571.

Magnetic Field - Gas Density Relation and Observational Implications Revisited

G. Panopoulou, V. Pavlidou, K. Tassis, 2015, 1505.05508.

Ambipolar Diffusion, Cloud Cores, and Star Formation: Two-dimensional, Cylindrically Symmetric Contraction. I. The Issues, Formulation of the Problem, and Method of Solution

S. Morton, T. Mouschovias, 1991 .

The Parker Instability in the Interstellar Medium

T. Mouschovias, 1996 .

Multifluid, Magnetohydrodynamic Shock Waves with Grain Dynamics. II. Dust and the Critical Speed for C Shocks

T. Mouschovias, W. Roberge, G. Ciolek, 2004, astro-ph/0404209.

The Magnetic Decoupling Stage of Star Formation

S. Desch, T. Mouschovias, 2001 .

Effect of Ambipolar Diffusion on Ion Abundances in Contracting Protostellar Cores

T. Mouschovias, G. Ciolek, 1998 .

Effect of Ambipolar Diffusion on Dust-to-Gas Ratio in Protostellar Cores

T. Mouschovias, G. Ciolek, 1996 .

Ambipolar Diffusion, Interstellar Dust, and the Formation of Cloud Cores and Protostars. II. Numerical Method of Solution

S. Morton, T. Mouschovias, G. Ciolek, 1994 .

Ambipolar diffusion, cloud cores, and star formation: Two-dimensional, cylindrically symmetric contraction, II. Results and a length scale for protostellar cores

S. Morton, T. Mouschovias, 1992 .

Ambipolar diffusion, cloud cores, and star formation: Two-dimensional, cylindrically symmetric contraction. III. A further parameter study and magnetically controlled accretion rate

S. Morton, T. Mouschovias, 1992 .

1 3 0 Se p 20 04 MAGNETICALLY-CONTROLED SPASMODIC ACCRETION DURING STAR FORMATION : I . FORMULATION OF THE PROBLEM AND METHOD OF SOLUTION

K. Tassis, T. Mouschovias, 2004 .

Molecular Cloud Cores and Protostars: Offsprings of Gravity and Cosmic Magnetism

T. Mouschovias, 1990 .

Multifluid Magnetohydrodynamics and Star Formation

T. Mouschovias, 1996 .

Role of Dust in Protostar Formation

T. Mouschovias, 1996 .

Star formation in magnetic interstellar clouds : II. Basic theory : how to manufacture stars by studying waves on strings

T. Mouschovias, 1987 .

Magnetic Braking and Angular Momenta of Protostars

T. Mouschovias, 1983 .

in The Origin of Stars and Planetary Systems

Telemachos Ch. Mouschovias, Glenn E. Ciolek, T. Mouschovias, 1999 .

The angular momentum problem during star formation Magnetically linked, aligned rotators. I - an exact, time-dependent solution

S. Morton, T. Mouschovias, 1985 .

The Angular Momentum Problem during Star Formation - Magnetically Linked Aligned Rotators - Part Two - Results

S. Morton, T. Mouschovias, 1985 .

Magnetically Controlled Spasmodic Accretion during Star Formation. I. Formulation of the Problem and Method of Solution

K. Tassis, T. Mouschovias, K. Tassis, 2004, astro-ph/0409769.

Magnetic braking of an aligned rotator during star formation: An exact, time-dependent solution

T. Mouschovias, E. Paleologou, 1980 .

Formation of interstellar cloud complexes, OB associations, and giant H II regions

P. Woodward, F. Shu, T. Mouschovias, 1974 .

THE NONISOTHERMAL STAGE OF MAGNETIC STAR FORMATION. I. FORMULATION OF THE PROBLEM AND METHOD OF SOLUTION

T. Mouschovias, M. Kunz, 2008, 0812.1791.

Magnetic Fields and Star Formation: A Theory Reaching Adulthood

Telemachos Ch. Mouschovias, Glenn E. Ciolek, T. Mouschovias, 1999 .

Observational Constraints on the Ages of Molecular Clouds and the Star Formation Timescale: Ambipolar-Diffusion-controlled or Turbulence-induced Star Formation?

K. Tassis, T. Mouschovias, M. Kunz, 2005, astro-ph/0512043.

Hydromagnetic Waves and the Linewidth-Size Relation in Interstellar Molecular Clouds

D. Psaltis, T. Mouschovias, 1995 .

Magnetically Controlled Spasmodic Accretion during Star Formation. II. Results

K. Tassis, T. Mouschovias, 2004, astro-ph/0410002.

Magnetic Braking, Ambipolar Diffusion, and the Formation of Cloud Cores and Protostars. II. A Parameter Study

S. D. James, S. Basu, A. R. Hyland, 1995 .

STRUCTURE AND EVOLUTION OF MAGNETICALLY SUPPORTED MOLECULAR CLOUDS : EVIDENCE FOR AMBIPOLAR DIFFUSION IN THE BARNARD 1 CLOUD

R. Crutcher, T. Troland, T. Mouschovias, 1994 .

Do lognormal column‐density distributions in molecular clouds imply supersonic turbulence?

H. Yorke, U. Illinois, J. Pineda, 2010, 1006.2826.