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

  title={A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary},
  author={Kishalay De and Mansi M. Kasliwal and Eran. O. Ofek and Takashi J. Moriya and Jamie Burke and Y. Cao and S. Bradley Cenko and G B Doran and Gina E. Duggan and Robert P. Fender and Claes Fransson and Avishay Gal-yam and Assaf Horesh and Shrinivas R. Kulkarni and Russ R. Laher and Ragnhild Lunnan and Ilan Manulis and Frank J. Masci and Paolo A. Mazzali and Peter E. Nugent and Daniel A. Perley and Tanja Petrushevska and Anthony L. Piro and Clare Rumsey and Jesper Sollerman and M. Sullivan and Francesco Taddia},
  pages={201 - 206}
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… 

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