Astronomy and Astrophysics – Astronomy
Scientist
Astronomy and Astrophysics
Astronomy
Scientist
Centro de Física, Instituto Venezolano de Investigaciones Científicas, Apartado 21827, Caracas 1020A, Venezuela
Instituto Nacional de Investigaciones Nucleares, ININ, Apartado Postal 18-1027, Mexico 11801 D.F.+International Centre for Theoretical Physics, ICTP, Strada Costiera 11, I-34014 Trieste, Italy
International School for Advanced Studies, SISSA, Strada Costiera 11, 34014 Trieste, Italy
Universidad de Los Andes, Merida, Venezuela
Instituto Venezolano de Investigaciones Científicas, IVIC, Apartado 21827, Caracas 1020A, Venezuela
Centro de Física, Instituto Venezolano de Investigaciones Científicas, IVIC, Apartado 21827, Caracas 1020A, Venezuela
Centro de Investigaciones de Astronomia, Merida, Venezuela
International Centre for Theoretical Physics; Scuola Internazionale di Studi Avanzati, Trieste, Italy
International Center for Theoretical Physics; Scuola Internazionale Superiore di Studi Avanzati, Trieste, Italy
Centro de Física, Instituto Venezolano de Investigaciones Científicas, IVIC, Apartado 21827, Caracas 1020A, Venezuela.
Centro de Fisica, Instituto Venezolano de Investigaciones Científicas, IVIC, Apartado 21827, Caracas, 1020A, Venezuela
Centro de Física, Instituto Venezolano de Investigaciones Científicas, Apartado Postal 21827, Caracas 1020A, Venezuela
Instituto Nacional de Investigaciones Nucleares, ININ Apartado Postal 18-1027, Mexico 11801 DF
Centro de Física, Instituto Venezolano de Investigaciones Científicas, IVIC, Apartado Postal 21827, Caracas 1020A, Venezuela Centre for Theoretical Physics; SISSA, Trieste, Italy
Catastrophic Cooling of Impulsively Heated Coronal Loops
Collapse and Fragmentation Models of Cloud Cores with Magnetic Field Support
Collapse and Fragmentation Models of Oblate Molecular Cloud Cores. III. Formation of Small Protostellar Clusters
Collapse and Fragmentation Models of Prolate Molecular Cloud Cores. I. Initial Uniform Rotation
Collapse and Fragmentation Models of Prolate Molecular Cloud Cores. II. Initial Differential Rotation
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