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

Konstantinos Tassis; Telemachos Ch. Mouschovias

doi:10.1086/424479

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

The Astrophysical Journal ◽

10.1086/424479 ◽

2005 ◽

Vol 618 (2) ◽

pp. 769-782 ◽

Cited By ~ 31

Author(s):

Konstantinos Tassis ◽

Telemachos Ch. Mouschovias

Keyword(s):

Star Formation ◽

Method Of Solution

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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

The Astrophysical Journal ◽

10.1086/154436 ◽

1976 ◽

Vol 206 ◽

pp. 753 ◽

Cited By ~ 130

Author(s):

T. Ch. Mouschovias

Keyword(s):

Star Formation ◽

Interstellar Clouds ◽

Method Of Solution ◽

Intercloud Medium

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

The Astrophysical Journal ◽

10.1086/171336 ◽

1992 ◽

Vol 391 ◽

pp. 199 ◽

Cited By ~ 60

Author(s):

Robert A. Fiedler ◽

Telemachos Ch. Mouschovias

Keyword(s):

Star Formation ◽

Ambipolar Diffusion ◽

Method Of Solution ◽

Cloud Cores

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The magnetic flux problem and ambipolar diffusion during star formation - One-dimensional collapse. I - Formulation of the problem and method of solution

The Astrophysical Journal ◽

10.1086/161578 ◽

1983 ◽

Vol 275 ◽

pp. 838 ◽

Cited By ~ 26

Author(s):

E. V. Paleologou ◽

T. Ch. Mouschovias

Keyword(s):

Star Formation ◽

Magnetic Flux ◽

Ambipolar Diffusion ◽

One Dimensional ◽

Method Of Solution

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ERRATUM: “THE NONISOTHERMAL STAGE OF MAGNETIC STAR FORMATION. I. FORMULATION OF THE PROBLEM AND METHOD OF SOLUTION” (2009, APJ, 693, 1895)

The Astrophysical Journal ◽

10.1088/0004-637x/696/2/2290 ◽

2009 ◽

Vol 696 (2) ◽

pp. 2290-2290

Author(s):

Matthew W. Kunz ◽

Telemachos Ch. Mouschovias

Keyword(s):

Star Formation ◽

Magnetic Star ◽

Method Of Solution

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Ambipolar diffusion, cloud cores, and star formation: Two-dimensional, cylindrically symmetric contraction. I - The issues, formulation of the problem, and method of solution

The Astrophysical Journal ◽

10.1086/169893 ◽

1991 ◽

Vol 371 ◽

pp. 296 ◽

Cited By ~ 39

Author(s):

Telemachos Ch. Mouschovias ◽

Scott A. Morton

Keyword(s):

Star Formation ◽

Ambipolar Diffusion ◽

Two Dimensional ◽

Cylindrically Symmetric ◽

Method Of Solution ◽

Cloud Cores

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

The Astrophysical Journal ◽

10.1088/0004-637x/693/2/1895 ◽

2009 ◽

Vol 693 (2) ◽

pp. 1895-1911 ◽

Cited By ~ 25

Author(s):

Matthew W. Kunz ◽

Telemachos Ch. Mouschovias

Keyword(s):

Star Formation ◽

Magnetic Star ◽

Method Of Solution

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Accretion Processes in Star Formation

10.1017/cbo9780511552090 ◽

2008 ◽

Cited By ~ 38

Author(s):

Lee Hartmann

Keyword(s):

Star Formation

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Cosmic dust charge shapes star formation

Nature India ◽

10.1038/nindia.2015.108 ◽

2015 ◽

Keyword(s):

Star Formation ◽

Cosmic Dust ◽

Dust Charge

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The role of interstellar filaments in shaping the IMF and regulating star formation

EAS Publications Series ◽

10.1051/eas/1575023 ◽

2015 ◽

Vol 75-76 ◽

pp. 137-141

Author(s):

P. André ◽

V. Könyves ◽

A. Roy

Keyword(s):

Star Formation ◽

The Imf

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Cosmological star formation history

EAS Publications Series ◽

10.1051/eas:2002046 ◽

2002 ◽

Vol 3 ◽

pp. 71-84

Author(s):

F. Hammer

Keyword(s):

Star Formation ◽

Star Formation History ◽

Formation History

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