Herschel observations of_the_w3_gmc_clues_to_the_formation_of_clusters_of_high_mass_stars
Nuria Marcelino (NRAO-CV) Molecular Line Surveys of Dark Clouds Discovery of CH 3 O.
A PROPER MOTION STUDY OF THE LUPUS CLOUDS B. López Martí (1), F. Jiménez Esteban (1,2) & E. Solano (1,2) (1) Centro de Astrobiología (INTA-CSIC); (2) Spanish.
New Young Stars (both human & astronomical) in the Gum Nebula
1 Enrique Vázquez-Semadeni Centro de Radioastronomía y Astrofísica, UNAM, México.
Introductory Overview Murray Lewis. Arecibo’s primary advantage is its unmatched sensitivity consequent on its large collecting area.
Chemical Enrichment and Outflows at z~1-6
Enrique Vázquez-Semadeni Centro de Radioastronomía y Astrofísica, UNAM, México
