A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary
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 wi...
Autors principals: | De, K, Kasliwal, MM, Ofek, EO, Moriya, TJ, Burke, J, Cao, Y, Cenko, SB, Doran, GB, Duggan, GE, Fender, RP, Fransson, C, Gal-Yam, A, Horesh, A, Kulkarni, SR, Laher, RR, Lunnan, R, Manulis, I, Masci, F, Mazzali, PA, Nugent, PE, Perley, DA, Petrushevska, T, Piro, AL, Rumsey, C, Sollerman, J, Sullivan, M, Taddia, F |
---|---|
Format: | Journal article |
Idioma: | English |
Publicat: |
American Association for the Advancement of Science
2018
|
Ítems similars
-
The subluminous and peculiar Type Ia supernova PTF09dav
per: Sullivan, M, et al.
Publicat: (2011) -
The Subluminous and Peculiar Type Ia Supernova PTF09dav
per: Sullivan, M, et al.
Publicat: (2011) -
The UV/optical spectra of the Type Ia supernova SN 2010jn: a bright supernova with outer layers rich in iron-group elements
per: Hachinger, S, et al.
Publicat: (2013) -
Supernova 2007bi as a pair-instability explosion.
per: Gal-Yam, A, et al.
Publicat: (2009) -
Search for Supernova Progenitor Stars with ZTF and LSST
per: Nora L. Strotjohann, et al.
Publicat: (2023-01-01)