Interacting supernovae from wide massive binary systems

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Volume 685 (May 2024)

A&A, 685 (2024) A58

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Table 2.

Data for observed SN-IIb progenitor stars, similarly to what has been reported in Yoon et al. (2017) and Sravan et al. (2020).

	From light-curves		From pre-explosion imaging
Name	$M_{env}^{ext}$ $M^{\mathrm{ext}}_{\mathrm{env}}$	R_LC	L	T_eff	R_BB	L	T_eff	R_BB
	(M_⊙)	(R_⊙)	(k L_⊙)	(kK)	(R_⊙)	(k L_⊙)	(kK)	(R_⊙)
1993J	^(a),(b) 0.15–0.40	/	^(c) $126_{- 62}^{+ 125}$ $126^{+125}_{-62}$	^(c) $4 . 27_{- 0.46}^{+ 0.52}$ $4.27^{+0.52}_{-0.46}$	$651_{- 221}^{+ 335}$ $651^{+335}_{-221}$	$155_{- 50}^{+ 74}$ $155^{+74}_{-50}$	$5 . 37_{- 0.24}^{+ 0.25}$ $5.37^{+0.25}_{-0.24}$	$455_{- 89}^{+ 110}$ $455^{+110}_{-89}$
2008ax	^(d),(*) (0.06)	^(d) 30–50	^(d) $49 . 0_{- 23.7}^{+ 151}$ $49.0^{+151}_{-23.7}$	^(d) $11 . 2_{- 3.6}^{+ 8.2}$ $11.2^{+8.2}_{-3.6}$	^(d) $58 . 9_{- 18.9}^{+ 11.1}$ $58.9^{+11.1}_{-18.9}$	$89 . 1_{- 35.4}^{+ 58.8}$ $89.1^{+58.8}_{-35.4}$	$14 . 5_{- 3.0}^{+ 3.7}$ $14.5^{+3.7}_{-3.0}$	$47 . 7_{- 19.5}^{+ 33.0}$ $47.7^{+33.0}_{-19.5}$
2011dh	^(f) 0.10	^(f),(g) 200–300	^(e) $88 . 1_{- 8.7}^{+ 9.6}$ $88.1^{+9.6}_{-8.7}$	^(e) $6 . 01_{- 0.27}^{+ 0.28}$ $6.01^{+0.28}_{-0.27}$	$274_{- 28}^{+ 31}$ $274^{+31}_{-28}$	$83 . 2_{- 28.2}^{+ 42.7}$ $83.2^{+42.7}_{-28.2}$	6.17 ± 0.01	$253_{- 47}^{+ 58}$ $253^{+58}_{-47}$
2013df	^(i),(†) 0.10–0.20	^(i),(†) 64–169	^(h) $87 . 1_{- 11.2}^{+ 12.9}$ $87.1^{+12.9}_{-11.2}$	^(h) 4.25 ± 0.10	$546_{- 44}^{+ 47}$ $546^{+47}_{-44}$	$74 . 1_{- 6.5}^{+ 7.2}$ $74.1^{+7.2}_{-6.5}$	4.37 ± 0.10	$477_{- 30}^{+ 32}$ $477^{+32}_{-30}$
2016gkg	^(j) 0.01–0.09	^(j) 300–340	^(j) $126_{- 45}^{+ 60}$ $126^{+60}_{-45}$	^(j) $7 . 25_{- 0.85}^{+ 0.90}$ $7.25^{+0.90}_{-0.85}$	^(j) $226_{- 73}^{+ 98}$ $226^{+98}_{-73}$	$191_{- 59}^{+ 85}$ $191^{+85}_{-59}$	$10 . 5_{- 2.3}^{+ 3.0}$ $10.5^{+3.0}_{-2.3}$	$133_{- 55}^{+ 95}$ $133^{+95}_{-55}$

Notes. Column 2 contains the estimated mass of the extended envelope, and Col. 3 shows the estimated progenitor radius, both as derived from light-curve modeling. Columns 4–6 show the estimated luminosity, effective temperature, and progenitor radius from pre-explosion imaging. Columns 7–9 summarize data for the pre-explosion properties of each progenitor as elaborated by Gilkis & Arcavi (2022), containing respectively the same quantity as in Cols. 4–6. ^( * )This value comes from one example binary evolution model which reproduces the L and T_eff of the pre-explosion image at the end of its evolution (Folatelli et al. 2015). ^( † )The source of these values uses the semi-analytical method presented in Nakar & Piro (2014).

References. (SN 1993J) ^(a)Woosley et al. (1994), ^(b)Houck & Fransson (1996) and ^(c) Maund et al. (2004; SN 2008ax) ^(d) Folatelli et al. (2015; SN 2011dh) ^(e)Maund et al. (2011), ^(f)Bersten et al. (2012) and ^(g) Ergon et al. (2015; SN 2013df) ^(h)Van Dyk et al. (2014) and ⁽ⁱ⁾ Morales-Garoffolo et al. (2014; SN 2016gkg) ^(j)Bersten et al. (2018).

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