Narrow transient absorptions in late-time optical spectra of type Ia supernovae: evidence for large clumps of iron-rich ejecta?
Author:
Affiliation:
1. Department of Physics and Astronomy, Dartmouth College, 6127 Wilder Lab, Hanover, NH 03755, USA
Funder
Dartmouth’s School
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/483/1/1114/27053295/sty3177.pdf
Reference85 articles.
1. Nucleosynthesis in Supernova Models. II. The ^{12}C Detonation Model
2. Progressive redshifts in the late-time spectra of Type Ia supernovae
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1. Understanding nebular spectra of Type Ia supernovae;Monthly Notices of the Royal Astronomical Society;2020-03-09
2. The Deepest Radio Observations of Nearby SNe Ia: Constraining Progenitor Types and Optimizing Future Surveys;The Astrophysical Journal;2020-02-25
3. A Nucleosynthetic Origin for the Southwestern Fe-rich Structure in Kepler’s Supernova Remnant;The Astrophysical Journal;2020-02-18
4. Constraining Type Ia supernova asymmetry with the gamma-ray escape time-scale;Monthly Notices of the Royal Astronomical Society;2019-05-08
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