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Title: A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary Authors: ID Petrushevska, Tanja (Author), et al. Files: This document has no files that are freely available to the public. This document may have a physical copy in the library of the organization, check the status via COBISS.  Language: English Work type: Not categorized Typology: 1.01 - Original Scientific Article Organization: UNG - University of Nova Gorica Abstract: 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 (≈0.2 solar masses) and low kinetic energy (≈2 × 1050 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. Keywords: supernova, neutron stars, gravitational waves Publication version: Author Accepted Manuscript Year of publishing: 2018 Number of pages: 201-206 Numbering: 6411, 362 PID: 20.500.12556/RUNG-4137-9b4c4fdc-31fd-77e4-5014-1991060ab100  COBISS.SI-ID: 5242619  DOI: 10.1126/science.aas8693  NUK URN: URN:SI:UNG:REP:1EVYHSK0 Publication date in RUNG: 12.10.2018 Views: 3291 Downloads: 0 Metadata:     Cite this work Plain text BibTeX EndNote XML EndNote/Refer RIS ABNT ACM Ref AMA APA Chicago 17th Author-Date Harvard IEEE ISO 690 MLA Vancouver : Copy citation

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Record is a part of a journal

Title:	ScienceScience
Publisher:	American Association for the Advancement of Science
Year of publishing:	2018
ISSN:	0036-80750193-4511

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