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The Radio Luminosity-Risetime Function of Core-Collapse Supernovae | Michael F. Bietenholz
; N. Bartel
; M. Argo
; R. Dua
; S. Ryder
; A. Soderberg
; | Date: |
23 Nov 2020 | Abstract: | We assemble a large set of 2-10 GHz radio flux density measurements and upper
limits of 294 different supernovae (SNe), from the literature and our own and
archival data. Only 31% of the SNe were detected. We characterize the SN
lightcurves near the peak using a two-parameter model, with $t_{
m pk}$ being
the time to rise to a peak and $L_{
m pk}$ the spectral luminosity at that
peak. Over all SNe in our sample at $D<100$ Mpc, we find that $t_{
m pk} =
10^{1.7pm0.9}$ d, and that $L_{
m pk} = 10^{25.5pm1.6}$ erg s$^{-1}$
Hz$^{-1}$, and therefore that generally, 50% of SNe will have $L_{
m pk} <
10^{25.5}$ erg s$^{-1}$ Hz$^{-1}$. These $L_{
m pk}$ values are ~30 times
lower than those for only detected SNe. Types I b/c and II (excluding IIn’s)
have similar mean values of $L_{
m pk}$ but the former have a wider range,
whereas Type IIn SNe have ~10 times higher values with $L_{
m pk} =
10^{26.5pm1.1}$ erg s$^{-1}$ Hz$^{-1}$. As for $t_{
m pk}$, Type I b/c have
$t_{
m pk}$ of only $10^{1.1pm0.5}$ d while Type II have $t_{
m pk} =
10^{1.6pm1.0}$ and Type IIn the longest timescales with $t_{
m pk} =
10^{3.1pm0.7}$ d. We also estimate the distribution of progenitor mass-loss
rates, $dot M$, and find the mean and standard deviation of log$_{10}(dot
M/$Msol) yr$^{-1}$ are $-5.4pm1.2$ (assuming $v_{
m wind}=1000$ km s$^{-1}$)
for Type I~b/c SNe, and $-6.9pm1.4$ (assuming $v_{
m wind} = 10$ km s$^{-1}$
for Type II SNe excluding Type IIn. | Source: | arXiv, 2011.11737 | Services: | Forum | Review | PDF | Favorites |
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