机译:由正中子星驱动的超发光X射线源
Universite de Toulouse, UPS-OMP, Institut de Recherche en Astrophysique et Planetologie, 9;
Avenue du Colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France,CNRS, Institut de Recherche en Astrophysique et Planetologie, 9, Avenue du Colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France;
Cahill Center for Astrophysics, 1216 East California Boulevard, California Institute of Technology, Pasadena, California 91125, USA;
Cahill Center for Astrophysics, 1216 East California Boulevard, California Institute of Technology, Pasadena, California 91125, USA;
Cahill Center for Astrophysics, 1216 East California Boulevard, California Institute of Technology, Pasadena, California 91125, USA;
MIT Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA;
Cahill Center for Astrophysics, 1216 East California Boulevard, California Institute of Technology, Pasadena, California 91125, USA;
Universite de Toulouse, UPS-OMP, Institut de Recherche en Astrophysique et Planetologie, 9;
Avenue du Colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France,CNRS, Institut de Recherche en Astrophysique et Planetologie, 9, Avenue du Colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France;
Physics Department, Columbia University, 538 West 120th Street, New York, New York 10027, USA;
Space Sciences Laboratory, University of California, Berkeley, California 94720, USA;
DTU Space, National Space Institute, Technical University of Denmark, Elektrovej 327, DK-2800 Lyngby, Denmark;
Lawrence Livermore National Laboratory, Livermore, California 94550, USA;
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 OHA, UK;
Columbia Astrophysics Laboratory, Columbia University, New York, New York 10027, USA;
NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA;
Department of Physics, McGill University, Montreal, Quebec H3A 2T8, Canada;
Cahill Center for Astrophysics, 1216 East California Boulevard, California Institute of Technology, Pasadena, California 91125, USA;
Department of Physics, Texas Tech University, Lubbock, Texas 79409, USA;
Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, Michigan 48109-1042, USA;
Cahill Center for Astrophysics, 1216 East California Boulevard, California Institute of Technology, Pasadena, California 91125, USA;
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA;
Cahill Center for Astrophysics, 1216 East California Boulevard, California Institute of Technology, Pasadena, California 91125, USA;
Space Sciences Laboratory, University of California, Berkeley, California 94720, USA;
Universite de Toulouse, UPS-OMP, Institut de Recherche en Astrophysique et Planetologie, 9;
Avenue du Colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France,CNRS, Institut de Recherche en Astrophysique et Planetologie, 9, Avenue du Colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France;
NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA;
机译:重新审视ULX光谱:吸收高磁化中子星,作为超发光X射线源的引擎
机译:聚集有中子星的超X射线源
机译:SMC?X-3:由具有非偶极子磁场的中子星驱动的最接近的超发光X射线源
机译:超光X射线源作为中子恒星,在高质量X射线二进制中以超临界速率推动和增强
机译:积聚的中子星和黑洞的X射线和光学观察以及恒星X射线旋光仪的构造和测试。
机译:M31中年轻的紧凑型物体:NuSTARChandra和Hubble的组合力量
机译:由正中子星驱动的超发光X射线源