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

De, K. (author)
Kasliwal, M. M. (author)
Ofek, E. O. (author)
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Moriya, T. J. (author)
Burke, J. (author)
Cao, Y. (author)
Cenko, S. B. (author)
Doran, G. B. (author)
Duggan, G. E. (author)
Fender, R. P. (author)
Fransson, Claes (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Gal-Yam, A. (author)
Horesh, A. (author)
Kulkarni, S. R. (author)
Laher, R. R. (author)
Lunnan, Ragnhild (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Manulis, I. (author)
Masci, F. (author)
Mazzali, P. A. (author)
Nugent, P. E. (author)
Perley, D. A. (author)
Petrushevska, Tanja (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC),University of Nova Gorica, Slovenia
Piro, A. L. (author)
Rumsey, C. (author)
Sollerman, Jesper (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Sullivan, M. (author)
Taddia, Francesco (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
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 (creator_code:org_t)
American Association for the Advancement of Science (AAAS), 2018
2018
English.
In: Science. - : American Association for the Advancement of Science (AAAS). - 0036-8075 .- 1095-9203. ; 362:6411, s. 201-206
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Compact neutron star binary systems are produced from binary massive stars through stellar evolution involving up to two supernova explosions. The final stages in the formation of these systems have not been directly observed. We report the discovery of iPTF 14gqr (SN 2014ft), a type Ic supernova with a fast-evolving light curve indicating an extremely low ejecta mass (approximate to 0.2 solar masses) and low kinetic energy (approximate to 2 x 10(50) ergs). Early photometry and spectroscopy reveal evidence of shock cooling of an extended helium-rich envelope, likely ejected in an intense pre-explosion mass-loss episode of the progenitor. Taken together, we interpret iPTF 14gqr as evidence for ultra-stripped supernovae that form neutron stars in compact binary systems.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Publication and Content Type

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art (subject category)

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