Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Galaxy Astrophysics
Scientist
Instituto de Astronomía y Meteorología, Av. Vallarta No. 2602, Col. Arcos Vallarta, C.P. 44130 Guadalajara, Jalisco, México
Instituto de Astronomía y Meteorología, Av. Vallarta No. 2602, Col. Arcos Vallarta, C.P. 44130 Guadalajara, Jalisco, Mexico
Instituto de Astronomía y Meteorología, Av Vallarta No. 2602, Col. Arcos Vallarta, C.P. 44130 Guadalajara, Jalisco, México
Heriot-Watt University, Edinburgh, UK
Instituto de Astronomia y Meteorologia, Av. Vallarta No. 2602, Col. Arcos Vallarta, C.P. 44130 Guadalajara, Jalisco, Mexico
Queen Mary College, London, England
Instituto de Astronomía y Meteorología, Av. Vallarte No. 2602, Col. Arcos Vallarte, C.P. 44130 Guadalajara, Jalisco, Mexico de Astrofisica de Canarias, La Laguna, Spain
Instituto de Astronomía y Meteorología, Av. Vallarta No. 2602, Col. Arcos Vallarta, CP 44130 Guadalajara, Jalisco, México
Instituto de Astronomía y Meteorología, Av. Vallarta No. 2602, Col. Arcos Vallarta, CP 44130 Guadalajara, Jalisco, Mexico
ESA, Astronomy Div., Noordwijk, Netherlands
ESA, European Space Research and Technology Centre, Noordwijk, Netherlands
Instituto de Astronomia y Meteorologia, Av. Vallarta No. 2602, Col. Arcos Vallarta, CP 44130 Guadalajara, Jalisco, Mexico
Instituto de Astronomia y Meteorologia, Avenida Vallarta 2602, Col. Arcos Vallarta, C.P. 44130 Guadalajara, Jalisco, Mexico
Instituto de Astronomia y Meteorologia, Avenida Vallarta 2602, Col. Arcos Vallarta, CP 44130 Guadalajara, Jalisco, Mexico
Instituto de Astronomía y Meteorología Universidad de Guadalajara, México
European Space Agency, Paris, France
Instituto de Astronomía y Meteorología, Avenida Vallarta 2602, Arcos Vallarta, C.P. 44130 Guadalajara, Jalisco, Mexico
Imperial College of Science and Technology, London, England
Instituto de Astronomía y Meteorología
2MASS near-infrared photometry of symbiotic stars
2MASS photometry of galactic planetary nebulae (Larios+, 2005)
A 1.4 GHz and 14.7 GHz Analysis of Density Gradients in Galactic Planetary Nebulae
A carbon star outflow envelope about IC 418
A CO J = 2-1 survey of type I post-main-sequence nebulae
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