Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Tel-Aviv U.
Tel Aviv U
Tel-Aviv University
Tel Aviv University
Tel Aviv and UC Berkeley
Tel Aviv U.
Tel Aviv University, Israel
School of Physics and Astronomy, Wise Observatory, Raymond and Beverly Sackler Faculty of Exact Sciences, Tel Aviv University, Ramat Aviv, Tel Aviv 69978, Israel
Max-Planck-Inst. für Physik und Astrophysik, Garching bei München, Germany
Max-Planck-Institut für Physik und Astrophysik, Garching bei München, Germany
Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany
School of Physics and Astronomy, Tel Aviv University, Ramat Aviv 69978, ISRAEL
School of Physics and Astronomy and the Wise Observatory, Beverly and Raymond Sackler Faculty of Exact Sciences, Tel Aviv University, Tel Aviv 69978, Israel School of Physics & Astronomy, Tel Aviv University, Israël
University of Tel Aviv
Tel Aviv University, Ramat Aviv, Israel
California Univ., Berkeley.
School of Physics and Astronomy, Tel Aviv University, Tel Aviv, Israel
Tel-Aviv University, Israel
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA
Physikalisches Inst. der Univ. zu Cologne, Cologne, Germany
Max-Planck-Institut für extraterrestrische Physik, München, Germany
Tel-Aviv University.
Tel Aviv Univ., Ramat Aviv, Israel
Tel Aviv University, School of Physics and Astronomy, Ramat Aviv, Israel
Institute for Advanced Study, Princeton, USA
Columbia University, New York; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA
Max-Planck-Institut für Physik und Astrophysik, Garching bei München, Germany; Tel Aviv University, Israel
School of Physics and Astronomy, Tel Aviv University
Tel Aviv University, Tel Aviv, Israel
A Close Look at Star Formation around Active Galactic Nuclei
A mid-infrared spectroscopic survey of starburst galaxies: excitation and abundances
A MIR Spectroscopic Survey of Starburst Galaxies
A Multiwavelength Study of 30 Doradus: The Interstellar Medium in a Low-Metallicity Galaxy
A PDR-Code Comparison Study
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Profile ID: LFWR-SCP-P-1007