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ABSENCE OF FAST-MOVING IRON IN AN INTERMEDIATE TYPE Ia SUPERNOVA BETWEEN NORMAL AND SUPER-CHANDRASEKHAR

Cao, Yi (author)
Johansson, J. (author)
Nugent, Peter E. (author)
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Goobar, Ariel (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Nordin, Jakob (author)
Kulkarni, S. R. (author)
Cenko, S. Bradley (author)
Fox, Ori D. (author)
Kasliwal, Mansi M. (author)
Fremling, Christoffer (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Amanullah, Rahman (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Hsiao, E. Y. (author)
Perley, D. A. (author)
Bue, Brian D. (author)
Masci, Frank J. (author)
Lee, William H. (author)
Chotard, Nicolas (author)
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 (creator_code:org_t)
2016
2016
English.
In: Astrophysical Journal. - 0004-637X .- 1538-4357. ; 823:2
  • Journal article (peer-reviewed)
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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