Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
UNAM
Inst. de Astronomia, UNAM, Mexico
Instituto de Ciencias Nucleares UNAM
UNAM, Mexico City
Instituto de Astronomia - Universidad Nacional Autonoma de Mexico
Instituto de Ciencias Nucleares, UNAM, Mexico
Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Apdo. Postal 70-543, CP: 04510, D. F., Mexico
Laboratorio de Química de Plasmas y Estudios Planetarios, Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Circuito Exterior, Ciudad Universitaria, Mexico City, Mexico
Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, México DF, México
Toronto, University, Canada
Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Ciudad Universitaria, Apartado Postal 70-543, CP 04510, México D. F., México de Ciencias Nucleares, Universidad Nacional Autónoma de México, Apartado Postal 70-543, CP 04510, México DF, Mexico Institute for Theoretical Astrophysics, Toronto, Canada
ICN-UNAM
Icn-Unam
ICN-UNAM, Mexico
ICNUNAM
Instituto de Ciencias Nucleares, UNAM, México
ICN-Unam
Inst. Astronomia, UNAM, Mexico DF
Instituto de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico
ICN UNAM
Instituto de Ciencias Nucleares, UNAM, Ap. 70-543, 04510 D.F., México de Ciencias Nucleares, Universidad Nacional Autónoma de México, Ap. 70-543, 04510 México, D.F., Mexico
Washington, University, Seattle
Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Apartado Postal 70-543, 04510 México D. F., México
Instituto de Astronomia, U.N.A.M.
IAUNAM
Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, 04510 D.F., México.
Instituto de Astronomia, Universidad Nacional Autonoma de Mexico, 04512 Mexico DF, Mexico
Mathematics Department, UMI
'Stromgren region' analysis of cometary H II regions
3-D Kinematics of the HH 110 jet
3D numerical simulations of a radiative Herbig-Haro jet in a supersonic side wind
3D numerical simulations of photodissociated and photoionized disks
3D Simulations of the Fragmentation of Photoevaporating Clumps Embedded in a Stellar Wind
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