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Table A.1

LMC remnants with a secured SN classification.

MCSNR Other name Age Evidencea Referencesb
(yr)

Core-collapse SNRs

J05366916 SNR 1987A 28 Historical Maggi et al. (2012b)
J05406920 B0540693 ~1600 Pulsar Kaaret et al. (2001)
J05256938 N132D ~3150 Ejecta, morphology Borkowski et al. (2007)
J05356602 N63A 20005000 Ejecta, Fe K Warren et al. (2003)
J05366913 22004900 Ejecta Kavanagh et al. (2015a)
J05056802 N23 ~4600 Ejecta, CCO, morphology Hughes et al. (2006)
J05266605 N49 ~4800 Ejecta, SGR, Fe K Park et al. (2012)
J05376910 N157B ~5000 c PWN Chen et al. (2006)
J05256559 N49B ~10000 Ejecta, morphology Park et al. (2003b)
J05366735 DEM L241 > 104 c HMXB Seward et al. (2012)
J04536829 B0453685 12 0001 5000 PWN, morphology Haberl et al. (2012a)
J05317100 N206 ~25 000 PWN candidate, morphology Williams et al. (2005)

Type Ia SNRs

J05096731 B0509675 400±120 Light echo, ejecta Rest et al. (2008)
Fe K, morphology

J05096844 N103B 860 Ejecta, Fe K Hughes et al. (1995)
J05196902 B0519690 600 ± 200 Ejecta, Fe K, morphology Hughes et al. (1995)
J05056753 DEM L71 ~4700 Ejecta. Fe K, morphology Hughes et al. (1998, 2003)
J05477025 B0548704 ~7100 Ejecta Hendrick et al. (2003), this work
J05346955 B0534699 ~10000 Ejecta, morphology Hendrick et al. (2003)
J05347033 DEM L238 ~13500 Ejecta Borkowski et al. (2006)
J05367039 DEM L249 ~15000 c Ejecta Borkowski et al. (2006)
J05067026 [HP99] 1139 17 00021 000 Ejecta Kavanagh et al. (in prep.), this work
J05086902 [HP99] 791 20 00025 000 Ejecta Bozzetto et al. (2014)
J05277104 [HP99] 1234 ~25 000 Ejecta Kavanagh et al. (2013), this work
J05476941 DEM L316A ~27 000c Ejecta Williams & Chu (2005)
J05116759 20 000 c Ejecta Maggi et al. (2014)
J05086830 20 000 c Ejecta Maggi et al. (2014)

Notes. Ages for the first three type Ia SNRs are from light echo measurements (Rest et al. 2005).

(a)

Morphology: Typed from X-ray morphology by Lopez et al. (2009, 2011). Fe K: Typed from the properties of the Fe K emission by Yamaguchi et al. (2014, see also Sect. 5.4. CCO: Central compact object. PWN: Pulsar wind nebula. SGR: Soft gamma-ray repeater.

(b)

Because of the multiple studies on most remnants, the given references are “see [...] and references therein”.

(c)

Uncertain age.

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