Astronomy:iPTF14atg

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Short description: Supernova event of May 2015 in constellation Coma Berenices

iPTF14atg
Other designationsiPTF 14atg
Spectral classIa
Date3 May 2015
Distance300 Mly (92 Mpc)
HostIC 831
Progenitor typeWhite dwarf

iPTF14atg is a type-Ia supernova discovered on 3 May 2015. The supernova is located in galaxy IC 831, some 300 Mly (92 Mpc) distant.[1] The supernova is thought to have ignited on May 2 or 3.[2] The supernova's shockwave slammed into a companion star, shocking it into producing an ultraviolet pulse.[3] The companion star that was hit is suspected to be a red giant star.[citation needed] This detection of the UV signal represents the first time the collision event of a supernova shockwave upon a companion star has been detected.[4] The supernova was discovered by the Intermediate Palomar Transient Factory (iPTF), a successor to the earlier Palomar Transient Factory, and based at the Palomar Observatory in California. The data was processed by collaborators in Europe, that lead to the supernova discovery.[3]

This single-degenerate white dwarf with normal star binary system represents one of two mechanisms for producing a type-Ia supernova, the other being double-degenerate two white dwarf binary stars.[1][4]

Further reading

  • Cao, Yi; Kulkarni, S. R; Howell, D. Andrew; Gal-Yam, Avishay; Kasliwal, Mansi M; Valenti, Stefano; Johansson, J; Amanullah, R et al. (2015). "A strong ultraviolet pulse from a newborn type Ia supernova". Nature 521 (7552): 328–31. doi:10.1038/nature14440. PMID 25993962. Bibcode2015Natur.521..328C. 

References

External links