Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Madrid-CSIC / INTA
DAMIR, CSIC, Madrid, Spain
Departamento de Astrofísica Molecular e Infrarroja, Instituto de Estructura de la Materia, CSIC, Serrano 121, E-28006 Madrid, Spain de Astrofísica Molecular e Infrarroja, Instituto de Estructura de la Materia, CSIC, Serrano 121, 28006 Madrid, Spain ; Observatorio Astronómico Nacional, Apartado 1143, 28800 Alcalá de Henares, Spain
DEMIRM, Observatoire de Paris, F-75014 Paris, France; Presently at NASA-Goddard Institute for Space Studies, 2880 Broadway, New York, USA
Departamento de Astrofísica Molecular e Infrarroja, Instituto de Estructura de la Materia, CSIC, Serrano 121, E-28006 Madrid, Spain
CSIC, IEM, Departamento de Física Molecular, Serrano 121, E-28006 Madrid, Spain; Division of Mathematics, Physics and Astronomy, MS 320-47, California Institute of Technology, Pasadena, CA 91125, USA
Centro de Astrobiología, CSIC-INTA, Madrid, Spain
DEMIRM / Observatoire de Paris-Meudon, 61 Avenue de l'Observatoire, F-75014 Paris, France; Observatorio Astronomico Nacional, Campus Universitario Apartado 1143, E-28800 Alcalade Henares, Madrid, Spain
DAMIR, CSIC, C. / Serrano 121, 28006 Madrid, Spain
Departamento de Astrofisica Molecular e Infrarroja, Instituto de Estructura de la Materia, CSIC, E-28006 Madrid, Spain.
Department Física Molecular, I.E.M., C.S.I.C, Serrano 121, E-28006 Madrid, Spain; Division of Physics, Mathematics and Astronomy, California Institute of Technology, MS 320-47, Pasadena, CA, 91125, USA
CAB. INTA-CSIC. Department of Astrophysics., Crta Torrejón km 4. Torrejón de Ardoz, Madrid, Spain
Instituto de Estructura de la Materia, Dpto de Física Molecular CSIC, Madrid, Spain
Instituto de Estructura de la Materia, Dpto de Astrofísica Molecular e Infrarroja CSIC, Madrid, Spain
Instituto de Estructura de la Materia, Departamento de Física Molecular, CSIC, Serrano 121, E-28006 Madrid, Spain; Division of Physics, Mathematics, and Astronom
28SiO in O-rich evolved stars (Pardo+ 1998)
28SiO v = 1 and v = 2, J = 1-0 maser variability in evolved stars. Eleven years of short spaced monitoring
A high resolution line survey of IRC+10216 with Herschel. First results: Detection of warm silicon dicarbide SiC2
A line confusion limited millimeter survey of Orion KL
A line confusion limited millimeter survey of Orion KL (I): sulfur carbon chains
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