The population of black widow pulsars

Autor: King, A. R., Beer, M. E., Rolfe, D. J., Schenker, K., Skipp, J. M.

Publikováno v: Mon.Not.Roy.Astron.Soc. 358 (2005) 1501-1504

We consider the population of black widow pulsars (BWPs). The large majority of these are members of globular clusters. For minimum companion masses < 0.1 Msun, adiabatic evolution and consequent mass loss under gravitational radiation appear to prov

Externí odkaz: http://arxiv.org/abs/astro-ph/0502511

How special is the Solar System?

Autor: Beer, M. E., King, A. R., Livio, M., Pringle, J. E.

Most mechanisms proposed for the formation of planets are modified versions of the mechanism proposed for the solar system. Here we argue that, in terms of those planetary systems which have been observed, the case for the solar system being a typica

Externí odkaz: http://arxiv.org/abs/astro-ph/0407476

After the Supernova: Runaway Stars and Massive X-ray Binary Populations with Metallicity.

Autor: Giménez, Àlvaro, Guinan, Edward, Niarchos, Panagiotis, Rucinski, Slavek, Dray, L. M., Dale, J. E., Beer, M. E., King, A. R., Napiwotzki, R.

Publikováno v: Close Binaries in the 21st Century: New Opportunities & Challenges; 2006, p277-280, 4p

After the Supernova: Runaway Stars and Massive X-ray Binary Populations with Metallicity.

Autor: Dray, L. M., Dale, J. E., Beer, M. E., King, A. R., Napiwotzki, R.

Publikováno v: Astrophysics & Space Science; Aug2006, Vol. 304 Issue 1-4, p279-282, 4p, 4 Graphs

A binary pulsar in a 53-minute orbit.

Autor: Pan Z; National Astronomical Observatories, Chinese Academy of Sciences, Beijing, People's Republic of China.; Guizhou Radio Astronomical Observatory, Guizhou University, Guiyang, People's Republic of China.; College of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People's Republic of China.; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, Beijing, People's Republic of China., Lu JG; National Astronomical Observatories, Chinese Academy of Sciences, Beijing, People's Republic of China.; Guizhou Radio Astronomical Observatory, Guizhou University, Guiyang, People's Republic of China.; College of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People's Republic of China.; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, Beijing, People's Republic of China., Jiang P; National Astronomical Observatories, Chinese Academy of Sciences, Beijing, People's Republic of China. pjiang@bao.ac.cn.; Guizhou Radio Astronomical Observatory, Guizhou University, Guiyang, People's Republic of China. pjiang@bao.ac.cn.; College of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People's Republic of China. pjiang@bao.ac.cn.; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, Beijing, People's Republic of China. pjiang@bao.ac.cn., Han JL; National Astronomical Observatories, Chinese Academy of Sciences, Beijing, People's Republic of China. hjl@bao.ac.cn.; College of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People's Republic of China. hjl@bao.ac.cn.; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, Beijing, People's Republic of China. hjl@bao.ac.cn., Chen HL; Yunnan Observatories, Chinese Academy of Sciences, Kunming, People's Republic of China., Han ZW; Yunnan Observatories, Chinese Academy of Sciences, Kunming, People's Republic of China.; University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People's Republic of China., Liu K; Max-Planck-Institut für Radioastronomie, Bonn, Germany., Qian L; National Astronomical Observatories, Chinese Academy of Sciences, Beijing, People's Republic of China.; Guizhou Radio Astronomical Observatory, Guizhou University, Guiyang, People's Republic of China.; College of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People's Republic of China.; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, Beijing, People's Republic of China., Xu RX; Department of Astronomy, Peking University, Beijing, People's Republic of China.; Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing, People's Republic of China.; State Key Laboratory of Nuclear Physics and Technology, School of Physics, Peking University, Beijing, People's Republic of China., Zhang B; Nevada Center for Astrophysics, University of Nevada, Las Vegas, NV, USA. bing.zhang@unlv.edu.; Department of Physics and Astronomy, University of Nevada, Las Vegas, NV, USA. bing.zhang@unlv.edu., Luo JT; National Time Service Center, Chinese Academy of Sciences, Xi'an, China., Yan Z; College of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People's Republic of China.; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, Beijing, People's Republic of China.; Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, People's Republic of China., Yang ZL; National Astronomical Observatories, Chinese Academy of Sciences, Beijing, People's Republic of China.; College of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People's Republic of China.; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, Beijing, People's Republic of China., Zhou DJ; National Astronomical Observatories, Chinese Academy of Sciences, Beijing, People's Republic of China.; College of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People's Republic of China.; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, Beijing, People's Republic of China., Wang PF; National Astronomical Observatories, Chinese Academy of Sciences, Beijing, People's Republic of China.; College of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People's Republic of China.; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, Beijing, People's Republic of China., Wang C; National Astronomical Observatories, Chinese Academy of Sciences, Beijing, People's Republic of China.; College of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People's Republic of China.; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, Beijing, People's Republic of China., Li MH; State Key Laboratory of Public Big Data, Guizhou University, Guiyang, People's Republic of China., Zhu M; National Astronomical Observatories, Chinese Academy of Sciences, Beijing, People's Republic of China.; Guizhou Radio Astronomical Observatory, Guizhou University, Guiyang, People's Republic of China.; College of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People's Republic of China.; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences, Beijing, People's Republic of China.

Publikováno v: Nature [Nature] 2023 Aug; Vol. 620 (7976), pp. 961-964. Date of Electronic Publication: 2023 Jun 20.