Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Bonn
AIfA / Bonn
School of Mathematics and Physics, University of Queensland
U Tokyo
Argelander Institute for Astronomy Bonn
Edinburgh
University of Queensland, Brisbane
RIKEN
AIfA, Bonn, Germany
Universität Bonn, Astronomische Institute, Germany
School of Mathematics and Physics, University of Queensland, Australia
Astronomisches Rechen-Institut Heidelberg, Moenchhofstrasse 12-14, D-69120 Heidelberg, Germany für Astronomie, Universität Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany
Astronomisches Rechen-Institut Heidelberg, Monchhofstrasse 12-14, D-69120 Heidelberg, Germany of Bonn, Argelander Institut for Astronomy, Germany
Sternwarte der Universität Bonn, Germany
Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany of Astronomy, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
University of Bonn, Bonn, Germany
Argelander Institute for Astronomy, University of Bonn
Queensland
Univ. of Tokyo
Argelander-Institut fuer Astronomie, Bonn, Germany
U.Bonn
AIfA, Bonn
AIfA, Bonn, Germany;
Sternwarte, University Bonn, Germany
UBonn
School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4068, Australia für Astronomie, Universität Bonn, Germany
Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121, Bonn, Germany für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
University of Tokyo
Argelander Institute for Astronomy, University of Bonn, Auf dem Hügel 71, 53121 Bonn, Germany
Argelander Institut für Astronomie, Rheinische Friedrich-W
A Comparison of ground-based Cepheid P-L Relations with HIPPARCOS Parallaxes
A comprehensive set of simulations studying the influence of gas expulsion on star cluster evolution
A Dynamical Model for the Globular Cluster G1
A Dynamical N-body Model for the Central Region of $ω$ Centauri
A new method to create initially mass segregated star clusters in virial equilibrium
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Profile ID: LFWR-SCP-P-12412