Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Bamberg
California Institute of Technology, Pasadena, CA 91125, USA
Caltech, Pasadena, CA 91125 USA
Dr. Karl Remeis-Observatory & ECAP, Astronomical Institute, Friedrich-Alexander University Erlangen-Nuremberg, Sternwartstr. 7, D-96049 Bamberg, Germany
Dr. Karl Remeis-Observatory & ECAP, Astronomical Institute, Friedrich-Alexander University, Erlangen-Nuremberg, Sternwartstr. 7, D-96049 Bamberg, Germany
Dr. Karl Remeis-Observatory & ECAP, Astronomical Institute, Friedrich-Alexander University, Erlangen-Nuremberg, Sternwartstr. 7, D 96049 Bamberg, Germany
Dr. Remeis Sternwarte Bamberg, Universität Erlangen-Nürnberg, Germany
Dr. Remeis-Sternwarte, Sternwartstr. 7, 96049 Bamberg, Germany Remeis-Sternwarte, Institute for Astronomy, University Erlangen-Nürnberg
Dr. Remeis Sternwarte, Astronomisches Institut & ECAP, University Erlangen-Nürnberg
Dr. Karl Remeis-Observatory & ECAP, University Erlangen-Nuremberg
Dr.-Remeis Sternwarte, Institute for Astronomy, University Erlangen-Nürnberg
Dr. Karl Remeis-Observatory & ECAP, Astronomical Institute, Friedrich-Alexander University Erlangen-Nuremberg, Sternwartstr. 7, D 96049 Bamberg, Germany
Dr.-Remeis-Sternwarte, Institute for Astronomy, University Erlangen-Nürnberg, Sternwartstr. 7, 96049 Bamberg, Germany Pasadena, CA, USA
Space Radiation Laboratory, California Institute of Technology, Pasadena, CA 91125.
10Be/9Be ratio up to 1.0 GeV/nucleon measured in the ISOMAX 98 balloon flight
2M0415+0154: a new bright, short-period subdwarf B pulsator
A measure of 10Be/9Be ratio above 1 GeV/nucleon: Results from the 1998 Flight of ISOMAX
AA Doradus and its Cool Companion - The Influence of Enhanced Metal Line Blanketing and the Reflection Effect
An EC 14026 pulsator in a reflection binary
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