Dust grains from the heart of supernovae | Astronomy & Astrophysics (A&A)

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Table 1

Observed and estimated physical properties of the four SNe compiled from the papers listed in column “Ref”.

SNR

Type

E_ex

⁵⁶Ni

M_prog

Age

n₀

M_dust

Ref.

⁵⁶Ni^mod

[10⁵¹ erg]

[M_⊙]

[Z_⊙]

[Years]

[cm^-3]

[M_⊙]

[10⁵¹ erg]

[M_⊙]

1987A

II^a

1.1

0.075^a

18−20^a

0.4

1.5

0.7−0.9

f, g, h

1.0

0.075

CasA

IIb^b

1−3

0.058−0.16^c

13−20^b

335

1.9

0.1−1

i, j, k

1.5

0.11

Crab

IIn-P^d

0.1

0.009−0.016^d

9−12^e

960

0.1−0.25

0.5

0.014

N49

1.8

N/A

18−20

0.4

4800

0.9

0.1−0.4

m, n

1.5

0.075

Notes. The last three columns indicate the input parameters used in the simulations.

Reference.

^(a)

Arnett et al. (1989);

^(b)

Krause et al. (2008);

^(c)

Eriksen et al. (2009);

^(d)

Smith (2013);

^(e)

MacAlpine & Satterfield (2008);

^(f)

Matsuura et al. (2011);

^(g)

Indebetouw et al. (2014);

^(h)

Lakićević et al. (2011);

⁽ⁱ⁾

Barlow et al. (2010);

^(j)

^(k)

^(l)

^(m)

⁽ⁿ⁾

Otsuka et al. (2010).

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