Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
IAA
IAA; Spain
IAA-CSIC
Instituto de Astrofísica de Andalucía, CSIC, Apdo. Postal 3004, E-18080, Granada, Spain
Instituto de Astrofísica de Andalucía, CSIC, Spain
Andalucia, Instituto de Astrofisica, Granada, Spain
Instituto de Astrofísica de Andalucía, Glorieta de la Astronomía s / n, Aptdo. 3004, 18080 Granada, Spain
Instituto de Astrofísica de Andalucía, CSIC, Apdo. 3004, E-18080 Granada, Spain de Astrofísica de Andalucía, CSIC, Apdo. Postal 3004, E-18080 Granada, Spain
Instituto de Astrofísica de Andalucía, CSIC, Apdo. 3004, E-18080, Granada, Spain
Andalucia, Inst. de Astrofisica, Granada, Spain; Boston University, MA
IAA.CSIC, Granada, Spain
Instituto de Astrofisica de Andalucia
Instituto de Astrofísica de Andalucía
Cadiz, Universidad, Cadiz; Consejo Superior de Investigaciones Cientificas, Instituto de Astrofisica de Andalucia, Granada, Spain
Consejo Superior de Investigaciones Cientificas, Instituto de Astrofisica de Andalucia, Granada; Sevilla, Universidad, Cadiz, Spain
Consejo Superior de Investigaciones Cientificas Instituto de Astrofisica de Andalucia, Granada; Cadiz, Universidad, Cadiz, Spain
Instituto de Astrofísica de Andalucía, Granada, Spain
Instituto de Astrofísica de Andalucía, Apdo. 3004, 18080, Granada, Spain
Instituto de Astrofísica de Andalucia, CSIC, Granada, Spain
Consejo Superior de Investigaciones Cientificas, Instituto de Astrofisica de Andalucia, Granada; Cadiz, Universidad, Cadiz, Spain; Basel, Universitat, Binningen, Switzerland
Instituto de Astrofísica de Andalucía, CSIC, Camino Bajo de Huétor 50, 18008, Granada, Spain de Astrofísica de Andalucía-CSIC, P.O. Box 3004, E-18080 Madrid, Spain
Instituto de Astrofísica de Andalucía-CSIC, Granada, Spain
6-m Telescope Spectroscopic Observations of The Bubble Complex in NGC 6946
A Metallicity Map of the Galactic Halo: Is There a Z -Abundance Gradient?
A non-parametric approach to the membership problem in open clusters
A photometric monitoring of bright high-amplitude delta Scuti stars. II. Period updates for seven stars
A Simple Method of Photographic Photometry Data Reduction
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