Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Astron. Inst., Univ. Basel
Astr. Inst., Univ. Basel
Astro. Inst. Univ. Basel
University of Basel, Switzerland
Astron.Inst., Univ. Basel
Department of Physics and Astronomy, Univ. of Basel
Astr. Inst. Univ. Basel
Department of Physics and Astronomy Basel
Astr. Institut Basel
Astronomical Institute of the University of Basel, Switzerland
Astr. Inst. Basel
Astronomisches Institut der Universitaet Basel
Dept. of Physics and Astronomy, Univ. of Basel, Switzerland
Astronomisches Institut der Universitaet Basel, Switzerland
Basel Universität, Basel, Switzerland; European Southern Observatory, Garching bei München, Germany
Astronomisches Institut, Basel, CH-4102, Switzerland
Astronomisches Institut der Universität Basel
Mount Wilson and Las Campanas Observatoires, Pasadena, CA
Mount Wilson and Las Campanas Observatoires, Pasadena, CA; Basel, Universität, Binningen, Switzerland
Basel, Universität, Switzerland; European Southern Observatory, Garching bei München, Germany
Basel Univ., Binningen, Switzerland
Basel, Universität, Basel; European Southern Observatory, Geneva, Switzerland
Hale Observatoires, Pasadena, Calif; Basel, Universität, Basel, Switzerland
Basel University
Basel, Universität, Basel, Switzerland; European Southern Observatory, Garching bei München, Germany
Basel Univ., Switzerland; ESO, Garching bei München, Germany
Hale Observatoires, Pasadena, Calif.
Basel, Universität, Binningen, Switzerland; European Southern Observatory, Garching bei München, Germany
Astronomisches Institut der Universität Bassel, Binningen, Switzerland
Astronomisches Institut der Universität Basel, Binningen, Switzerland
Hale Observatoires, Pasadena, Calif; Basel, Universität, Binningen, Switzerland
ESO
Basel Univ., Binningen, Switzerland; ESO, Garching bei München, Germany
European Southern Observatory, Geneva; Basel
21 centimeter line width distances of cluster galaxies and the value of H0
A Case for the Standard Model
A Composite Period-Luminosity Relation for Cepheids at Mean and Maximum Light
A New Method to Derive the Distances of Spiral Galaxies
A Possible Identification of the X-ray Source Sco X-3
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Profile ID: LFWR-SCP-P-95153