Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
N. Copernicus Astronomical Center
N. Copernicus Astronomical Center, Warsaw, Poland
Warsaw University Observatory and N. Copernicus Astronomical Centre
Warsaw University Observatory, Al. Ujazdowskie 4, PL-00478 Warszawa, Poland
Obserwatorium Astronomiczne, Warsaw, Poland
University of Warsaw Observatory, Warsaw, Poland
Warsaw Univ. Observatory, Poland
Warsaw University, and Nicolaus Copernicus Center
for the Pi of the Sky collaboration
Nicolaus Copernicus Astronomical Center, Warsaw, Poland
Max-Planck-Institut für Astrophysik, Garching bei München, Germany; Warszawa, Uniwersytet, Obserwatorium Astronomiczne, Warsaw, Poland
University of California Observatoires / Lick Observatory, Board of Studies in Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064
Copernicus Astronomical Center, Poland
Max-Planck-Institut für Physik und Astrophysik, Garching bei München, Germany; Obserwatorium Astronomiczne, Warsaw, Poland; Lick Observatory, Santa Cruz, CA
Warsaw University Observatory, Al. Ujazdowskie 4, Pl-00478 Warszawa, Poland
University Observatory, Warsaw, Poland
Max-Planck-Institut für Physik und Astrophysik, Munich, Germany
Warsaw University Observatory;, Max-Planck-Institut für Astrophysik
Warsaw, University, Observatory, Poland
Nicolaus Copernicus Astronomical Center, Bartycka 18, Warsaw, 00-716, Poland Observatory, Santa Cruz, CA
Lick Observatory, Santa Cruz, CA; Obserwatorium Astronomiczne, Warsaw, Poland
Nicolaus Copernicus Astronomical Center, Bartycka 18, Warsaw 00-716, Poland
Warsaw Univ. Observatory, Poland; Inst. de Astrofisica de Canarias, La Laguna, Spain
University of California Observatoires / Lick Observatory, University of California, Santa Cruz, CA 95064; Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warszawa, Poland Astronomiczne, Warsaw, Poland; Max-Planck-Institut für Ph
2-D models of layered protoplanetary discs: I. The ring instability
2D Simulations of Stellar Convection. II. A Study of the Dependence of the Results on Numerical Methods
3-D simulations of the collapse of nonspherical interstellar clouds
A New Lower Main Sequence Eclipsing Binary with Detached Components
A Numerical Study of Magnetic Buoyancy in an Accretion Disk
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