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ABSENCE OF FAST-MOV...
ABSENCE OF FAST-MOVING IRON IN AN INTERMEDIATE TYPE Ia SUPERNOVA BETWEEN NORMAL AND SUPER-CHANDRASEKHAR
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Cao, Yi (author)
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Johansson, J. (author)
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Nugent, Peter E. (author)
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- Goobar, Ariel (author)
- Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
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Nordin, Jakob (author)
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Kulkarni, S. R. (author)
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Cenko, S. Bradley (author)
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Fox, Ori D. (author)
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Kasliwal, Mansi M. (author)
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- Fremling, Christoffer (author)
- Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
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- Amanullah, Rahman (author)
- Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
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Hsiao, E. Y. (author)
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Perley, D. A. (author)
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Bue, Brian D. (author)
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Masci, Frank J. (author)
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Lee, William H. (author)
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Chotard, Nicolas (author)
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(creator_code:org_t)
- 2016
- 2016
- English.
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In: Astrophysical Journal. - 0004-637X .- 1538-4357. ; 823:2
- Related links:
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https://urn.kb.se/re...
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https://doi.org/10.3...
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Abstract
Subject headings
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- In this paper, we report observations of a peculiar SN Ia iPTF13asv (a.k.a., SN2013cv) from the onset of the explosion to months after its peak. The early-phase spectra of iPTF13asv show an absence of iron absorption, indicating that synthesized iron elements are confined to low-velocity regions of the ejecta, which, in turn, implies a stratified ejecta structure along the line of sight. Our analysis of iPTF13asv's light curves and spectra shows that it is an intermediate case between normal and super-Chandrasekhar events. On the one hand, its light curve shape (B-band Delta m(15)=1.03 +/- 0.01) and overall spectral features resemble those of normal SNe Ia. On the other hand, its large peak optical and UV luminosity (M-B = -19.84 mag, M-uvm2 = -15.5 mag) and its low but almost constant Si II velocities of about 10,000 km s (1) are similar to those in super-Chandrasekhar events, and its persistent carbon signatures in the spectra are weaker than those seen commonly in super-Chandrasekhar events. We estimate a Ni-56 mass of 0.81(-0.18)(+0.10) M-circle dot and a total ejecta mass of 1.59(-0.12)(+0.45) M-circle dot. The large ejecta mass of iPTF13asv and its stratified ejecta structure together seemingly favor a double-degenerate origin.
Subject headings
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Keyword
- supernovae: general
- supernovae: individual (iPTF13asv)
- ultraviolet: general
Publication and Content Type
- ref (subject category)
- art (subject category)
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- By the author/editor
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Cao, Yi
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Johansson, J.
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Nugent, Peter E.
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Goobar, Ariel
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Nordin, Jakob
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Kulkarni, S. R.
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show more...
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Cenko, S. Bradle ...
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Fox, Ori D.
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Kasliwal, Mansi ...
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Fremling, Christ ...
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Amanullah, Rahma ...
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Hsiao, E. Y.
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Perley, D. A.
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Bue, Brian D.
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Masci, Frank J.
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Lee, William H.
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Chotard, Nicolas
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show less...
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- NATURAL SCIENCES
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NATURAL SCIENCES
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and Physical Science ...
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and Astronomy Astrop ...
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Astrophysical Jo ...
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Stockholm University