...
机译:脉冲星计时的引力波极限限制了超大质量黑洞的演化
Commonwealth Scientific and Industrial Research Organisation (CSIRO) Astronomy and Space Science, Australia Telescope National Facility, Post Office Box 76, Epping, New South Wales 1710, Australia;
Commonwealth Scientific and Industrial Research Organisation (CSIRO) Astronomy and Space Science, Australia Telescope National Facility, Post Office Box 76, Epping, New South Wales 1710, Australia,School of Physics, University of Melbourne, Parkville, Victoria 3010, Australia;
Department of Electrical and Computer Engineering, University of California at San Diego, La Jolla, CA 92093, USA;
Commonwealth Scientific and Industrial Research Organisation (CSIRO) Astronomy and Space Science, Australia Telescope National Facility, Post Office Box 76, Epping, New South Wales 1710, Australia;
Commonwealth Scientific and Industrial Research Organisation (CSIRO) Astronomy and Space Science, Australia Telescope National Facility, Post Office Box 76, Epping, New South Wales 1710, Australia;
Commonwealth Scientific and Industrial Research Organisation (CSIRO) Astronomy and Space Science, Australia Telescope National Facility, Post Office Box 76, Epping, New South Wales 1710, Australia;
School of Physics, University of Melbourne, Parkville, Victoria 3010, Australia;
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Post Office Box 218, Hawthorn, Victoria 3122, Australia;
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Post Office Box 218, Hawthorn, Victoria 3122, Australia,International Centre for Radio Astronomy Research, Curtin University, Bentley, Western Australia 6102, Australia;
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109-8099, USA;
Commonwealth Scientific and Industrial Research Organisation (CSIRO) Astronomy and Space Science, Australia Telescope National Facility, Post Office Box 76, Epping, New South Wales 1710, Australia,CSIRO Advanced Scientific Computing, Information Management and Technology, Private Bag 33, Clayton, Victoria 3169, Australia;
School of Physics, Monash University, Post Office Box 27, Victoria 3800, Australia;
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Post Office Box 218, Hawthorn, Victoria 3122, Australia;
CSIRO Astronomy and Space Science, Parkes Observatory, Post Office Box 276, Parkes, New South Wales 2870, Australia;
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Post Office Box 218, Hawthorn, Victoria 3122, Australia;
Max-Planck-lnstitut fuer Radioastronomie, Auf dem Hiigel 69, 53121 Bonn, Germany;
Commonwealth Scientific and Industrial Research Organisation (CSIRO) Astronomy and Space Science, Australia Telescope National Facility, Post Office Box 76, Epping, New South Wales 1710, Australia,Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi, Xinjiang 830011, China;
机译:利用脉冲运动时序阵列约束星系和超大黑洞二元合并的天体物理观察
机译:利用PULSAR时序控制超大规模黑洞双星的相变速率
机译:使用脉冲正时约束超大规模黑洞系统的属性:在3C 66B中的应用
机译:限制3C66B中提出的超大型黑洞系统的特性:脉冲节定时的限制
机译:用统计类星体样本约束超大质量黑洞的宇宙演化。
机译:硬X射线观测揭示银河系中心超大质量黑洞的宇宙学演化
机译:脉冲星定时约束超大质量的引力波极限 黑洞演变
机译:在3C66B中约束所提出的超大质量黑洞系统的性质:来自脉冲星定时的限制