Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
CRyA-UNAM, Morelia, Mexico
Instituto de Astronomia, UNAM, Unidad Morelia, Mexico
CRyA, UNAM, Mexico
Centro de Radioastronomía y Astrofísica, UNAM, Campus Morelia, C.P. 58090 Morelia, Michoacán, México
Leeds, University, England
Universidad Nacional Autonoma de Mexico, Mexico
Instituto de Astronomía, UNAM, Morelia
Centro de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Campus Morelia, Apartado Postal 3-72, 58090, Morelia, Michoacán, México
Instituto de Astronomía, U. Nacional Autónoma de México
Instituto de Astronomía, Universidad Nacional Autónoma de México, J. J. Tablada 1006, Colonia Lomas de Santa Maria, 58090 Morelia, Michoacán, México de Astronomía, UNAM, J. J. Tablada 1006, 58090 Morelia, Michoacán, México
Manchester Victoria Univ., United Kingdom
Instituto de Astronomía, UNAM
Instituto de Astronomia, UNAM, Campus Morelia, Apartado Postal 3-72, 58090 Morelia, Michoacán, Mexico
Manchester, Victoria Univ., United Kingdom
Centro de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Apdo. Postal 3-72, 58090 Morelia, Michoacán, México
Instituto de Ast ronomia, U.N.A.M., Morelia
Centro de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Campus Morelia, Apartado Postal 3-72, 58090 Morelia, Michoacán, México; On sabbatical leave at the Department of Physics and Astronomy, University of Leeds, Woodhouse Lane, Leeds LS2 9JT, UK.
Instituto de Astronomía, UNAM, Morelia, Michoacán, México
Centro de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Apartado Postal 3-72, 58090 Morelia, México
3D Transfer of the Diffuse Ionizing Radiation in ISM Flows and the Preionization of a Herbig-Haro Working Surface
A coupled hydrodynamic-ionisation model for the clumpy Wolf-Rayet ring nebula RCW 58.
Astrophysical Plasmas: Codes, Models, and Observations
Dynamical HII Region Evolution in Turbulent Molecular Clouds
Dynamics of Bubbles in the ISM
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