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Results 1 to 20 of 38 for query "E. Vazquez-Semadeni ". (0.01 sec.)

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A Turbulent Model for the Interstellar Medium. II. Magnetic Fields and Rotation
T. Passot; E. Vazquez-Semadeni; A. Pouquet;
30 Dec 1995 / ApJ 455, 536

Emissivity Statistics in Turbulent, Compressible MHD Flows and the Density-Velocity Correlation
Alex Lazarian; Dmitri Pogosyan; Enrique Vazquez-Semadeni; Barbara Pichardo;
22 Feb 2001

Density probability distribution in one-dimensional polytropic gas dynamics
Thierry Passot; Enrique Vazquez-Semadeni;
10 Feb 1998

The Lifetimes of Molecular Cloud Cores: What is the Role of the Magnetic Field?
E. Vazquez-Semadeni; J. Kim; M. Shadmehri; J. Ballesteros-Paredes;
5 Mar 2004

Molecular cloud evolution. I. Molecular cloud and thin CNM sheet formation
Enrique Vazquez-Semadeni; Dongsu Ryu; Thierry Passot; Ricardo F. Gonzalez; Adriana Gazol;
6 Sep 2005

The Lifetimes and Evolution of Molecular Cloud Cores
Enrique Vazquez-Semadeni; Jongsoo Kim; Mohsen Shadmehri; Javier Ballesteros-Paredes;
10 Sep 2004 / Astrophys.J. 618 (2004) 344-359

Compressible MHD Turbulence: Implications for Molecular Cloud and Star Formation
E. Vazquez-Semadeni; E. C. Ostriker; T. Passot.; C. F. Gammie; J. M. Stone;
3 Mar 1999

Turbulent Control of the Star Formation Efficiency
Enrique Vazquez-Semadeni;
23 Sep 2004

Influence of Cooling-Induced Compressibility on the Structure of Turbulent Flows and Gravitational Collapse
E. Vazquez-Semadeni; T. Passot; A. Pouquet;
9 Jul 1996

10.

A Holistic Scenario of Turbulent Molecular Cloud Evolution and Control of the Star Formation Efficiency. First Tests
E. Vazquez-Semadeni; J. Ballesteros-Paredes; R. S. Klessen;
28 Dec 2002 / Astrophys.J. 585 (2003) L131-L134

11.

Can Hydrostatic Cores Form Within Isothermal Molecular Clouds?
Enrique Vazquez-Semadeni; Mohsen Shadmehri; Javier Ballesteros-Paredes;
13 Aug 2002

12.

Velocity Structure of the ISM as Seen by the Spectral Correlation Function
Javier Ballesteros-Paredes; Enrique Vazquez-Semadeni; Alyssa A. Goodman;
4 Apr 2002

13.

The nonlinear development of the thermal instability in the atomic ISM and its interaction with random fluctuations
F.J. Sanchez-Salcedo; E. Vazquez-Semadeni; A. Gazol;
6 Mar 2002 / Astrophys.J. 577 (2002) 768-788

14.

Thermal Instability and Magnetic Pressure in the Turbulent ISM
Enrique Vazquez-Semadeni; Adriana Gazol; Thierry Passot; Javier Sanchez-Salcedo;
31 Dec 2001 / Lect.Notes Phys. 614 (2003) 213-251

15.

The Probability Distribution Function of Column Density in Molecular Clouds
Enrique Vazquez-Semadeni; Nieves Garcia;
14 Mar 2001

16.

The Density Probability Distribution Function in Turbulent, Isothermal, Magnetized Flows in Slab Geometry
Enrique Vazquez-Semadeni; Thierry Passot;
5 Nov 2000

17.

Does Turbulent Pressure Behave as a Logatrope?
E. Vazquez-Semadeni; J. Canto & S. Lizano;
15 Aug 1997

18.

A Search for Larson-Type Relations in Numerical Simulations of the ISM. Evidence for Non-Constant Column Densities
E. Vazquez-Semadeni; J. Ballesteros-Paredes & L.F. Rodriguez;
1 Aug 1996

19.

MHD Turbulence, Cloud Formation and Star Formation in the ISM
E. Vazquez-Semadeni; T. Passot; A. Pouquet;
1 Feb 1996 / Proc. "The Fifth Mexico-Texas Conference on Astrophysics: Gaseous Nebulae and Star Formation", Rev. Mex. Astr. Ap. Ser. Conf. 3, 61 (1995)

20.

Cloud Statistics in Numerical Simulations of the ISM
J. Ballesteros-Paredes; E. Vazquez-Semadeni;
1 Feb 1996 / Proc. "The Fifth Mexico-Texas Conference on Astrophysics: Gaseous Nebulae and Star Formation", Rev. Mex. Astr. Ap. Ser. Conf. 3, 105 (1995)

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