A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary-Reference-Cited by-同舟云学术

A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary

Published:2018-10-12 Issue:6411 Volume:362 Page:201-206
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

De K.¹^ORCID,Kasliwal M. M.¹^ORCID,Ofek E. O.²,Moriya T. J.³^ORCID,Burke J.⁴⁵,Cao Y.⁶,Cenko S. B.⁷⁸^ORCID,Doran G. B.⁹^ORCID,Duggan G. E.¹^ORCID,Fender R. P.¹⁰,Fransson C.¹¹^ORCID,Gal-Yam A.²,Horesh A.¹²^ORCID,Kulkarni S. R.¹^ORCID,Laher R. R.¹³,Lunnan R.¹¹^ORCID,Manulis I.²,Masci F.¹³,Mazzali P. A.¹⁴¹⁵^ORCID,Nugent P. E.¹⁶¹⁷^ORCID,Perley D. A.¹⁴^ORCID,Petrushevska T.¹⁸¹⁹^ORCID,Piro A. L.²⁰,Rumsey C.²¹,Sollerman J.¹¹^ORCID,Sullivan M.²²^ORCID,Taddia F.¹¹^ORCID

Affiliation:

1. Cahill Centre for Astrophysics, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA.

2. Department of Particle Physics and Astrophysics, Faculty of Physics, The Weizmann Institute of Science, Rehovot 76100, Israel.

3. Division of Theoretical Astronomy, National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan.

4. Las Cumbres Observatory, 6740 Cortona Drive, Suite 102, Goleta, CA 93117, USA.

5. Department of Physics, University of California, Santa Barbara, CA 93106, USA.

6. Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195, USA.

7. Astrophysics Science Division, NASA Goddard Space Flight Center, Mail Code 661, Greenbelt, MD 20771, USA.

8. Joint Space-Science Institute, University of Maryland, College Park, MD 20742, USA.

9. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.

10. Department of Physics, Astrophysics, University of Oxford, Denys Wilkinson Building, Oxford OX1 3RH, UK.

11. Oskar Klein Centre, Department of Astronomy, Stockholm University, 106 91 Stockholm, Sweden.

12. Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem 91904, Israel.

13. Infrared Processing and Analysis Center, California Institute of Technology, MS 100-22, Pasadena, CA 91125, USA.

14. Astrophysics Research Institute, Liverpool John Moores University, Liverpool L3 5RF, UK.

15. Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85748 Garching bei München, Germany.

16. Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA.

17. Department of Astronomy, University of California, Berkeley, CA, 94720, USA.

18. Oskar Klein Centre, Department of Physics, Stockholm University, 106 91 Stockholm, Sweden.

19. Centre for Astrophysics and Cosmology, University of Nova Gorica, Vipavska 11c, 5270 Ajdovščina, Slovenia.

20. The Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101, USA.

21. Astrophysics Group, Cavendish Laboratory, 19 J J Thomson Avenue, Cambridge CB3 0HE, UK.

22. Department of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK.

Abstract

Explosive origin of a binary neutron star Some types of core-collapse supernovae are known to produce a neutron star (NS). A binary NS merger was recently detected from its gravitational wave emission, but it is unclear how such a tight binary system can be formed. De et al. discovered a core-collapse supernova with unusual properties, including the removal of the outer layers of the star before the explosion. They interpret this as the second supernova in an interacting binary system that already contains one NS. Because the explosion probably produced a second NS (rather than a black hole) in a tight orbit, it could be an example of how binary NS systems form. Science , this issue p. 201

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference179 articles.

1. The evolution and explosion of massive stars

2. Progenitors of Core-Collapse Supernovae

3. Presupernova Evolution of Massive Single and Binary Stars

4. Binary Interaction Dominates the Evolution of Massive Stars

5. TYPE Ib/c SUPERNOVAE IN BINARY SYSTEMS. I. EVOLUTION AND PROPERTIES OF THE PROGENITOR STARS

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