Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Universidad Nacional Autónoma de México, México
DAEC, Obs. Meudon
UNAM
Instituto de Astronomía, Universidad Nacional Autónoma de México, Ensenada, CP 22800, Baja California, Mexico
OAN, Instituto de Astronomi UNAM, P.O. Box 439027, San Diego, CA, USA 92143
Instituto de Astronomía, Universidad Nacional Autónoma de México, Ensenada, México
Instituto de Astronomia, U.N.A.M.
DAEC, Observatoire de Meudon, F-92195 Meudon Cedex, France
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apartado Postal 877, 22800 Ensenada, Baja California, México
Instituto de Astronómia, UNAM, Campus Ensenada, Apartado Postal 877, 22800 Ensenada, Mexico
Instituto de Astronomía, Universidad Nacional Autónoma de México, Campus Ensenada, Ensenada, Baja California, 22800, Mexico
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 877, Ensenada, BC, Mexico
Instituto de Astronomia, Universidad Nacional Autonoma de Mexico, Apdo. Postal 70 264, Mexico D.F. 04510, Mexico de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 877, 22800 Ensenada, Baja California, Mexico
Instituto de Astronomía, UNAM
Observatorio Astronomico Nacional, PO Box 439027, San Diego, CA 92143-9027, USA
David Dunlap Observatory, Richmond Hill, Canada
IAUNAM, Mexico City
Observatorio Astronomico Nacional, UNAM, Mexico
York University, North York, Canada
Toronto, University, Canada
Mount Stromlo and Siding Spring Observatory, Canberra, Australia
Ctr. for Research in Earth & Space Science, York Univ., North York, Canada
Instituto de Astronomía, Universidad Autónoma de México, P.O. Box 439027, San Diego, CA 92143, USA
York Univ., North York, Canada
A catalog of planetary nebula candidates and HII regions in NGC 3109
A close binary nucleus in the most oxygen-poor planetary nebula PN G 135.9+55.9
A Wide Field Survey of Planetary Nebulae in M31: A Progress Report
Bright Planetary Nebulae and their Progenitors in Galaxies Without Star Formation
Bright planetary nebulae as probes of chemical evolution
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