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Stellar dynamics. The fastest unbound star in our Galaxy ejected by a thermonuclear supernova.
Geier, S; Fürst, F; Ziegerer, E; Kupfer, T; Heber, U; Irrgang, A; Wang, B; Liu, Z; Han, Z; Sesar, B; Levitan, D; Kotak, R; Magnier, E; Smith, K; Burgett, W S; Chambers, K; Flewelling, H; Kaiser, N; Wainscoat, R; Waters, C.
Afiliação
  • Geier S; European Southern Observatory, Karl-Schwarzschild-Straße 2, 85748 Garching, Germany. Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics, Astronomical Institute, Friedrich-Alexander University Erlangen-Nuremberg, Sternwartstraße 7, 96049 Bamberg, Germany. sgeier@eso.org.
  • Fürst F; Space Radiation Lab, MC 290-17 Cahill, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA.
  • Ziegerer E; Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics, Astronomical Institute, Friedrich-Alexander University Erlangen-Nuremberg, Sternwartstraße 7, 96049 Bamberg, Germany.
  • Kupfer T; Department of Astrophysics/Institute for Mathematics, Astrophysics and Particle Physics, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, Netherlands.
  • Heber U; Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics, Astronomical Institute, Friedrich-Alexander University Erlangen-Nuremberg, Sternwartstraße 7, 96049 Bamberg, Germany.
  • Irrgang A; Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics, Astronomical Institute, Friedrich-Alexander University Erlangen-Nuremberg, Sternwartstraße 7, 96049 Bamberg, Germany.
  • Wang B; Key Laboratory of the Structure and Evolution of Celestial Objects, Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China.
  • Liu Z; Key Laboratory of the Structure and Evolution of Celestial Objects, Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China. Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany.
  • Han Z; Key Laboratory of the Structure and Evolution of Celestial Objects, Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China.
  • Sesar B; Division of Physics, Mathematics, and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA. Max-Planck-Institut für Astronomie, Königstuhl 17, 69117, Heidelberg, Germany.
  • Levitan D; Division of Physics, Mathematics, and Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA.
  • Kotak R; Astrophysics Research Center, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, UK.
  • Magnier E; Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA.
  • Smith K; Astrophysics Research Center, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, UK.
  • Burgett WS; Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA.
  • Chambers K; Max-Planck-Institut für Astronomie, Königstuhl 17, 69117, Heidelberg, Germany.
  • Flewelling H; Max-Planck-Institut für Astronomie, Königstuhl 17, 69117, Heidelberg, Germany.
  • Kaiser N; Max-Planck-Institut für Astronomie, Königstuhl 17, 69117, Heidelberg, Germany.
  • Wainscoat R; Max-Planck-Institut für Astronomie, Königstuhl 17, 69117, Heidelberg, Germany.
  • Waters C; Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA.
Science ; 347(6226): 1126-8, 2015 Mar 06.
Article em En | MEDLINE | ID: mdl-25745168

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Science Ano de publicação: 2015 Tipo de documento: Article País de afiliação: Alemanha

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Science Ano de publicação: 2015 Tipo de documento: Article País de afiliação: Alemanha