Table A.1
LMC remnants with a secured SN classification.
MCSNR | Other name | Age | Evidencea | Referencesb |
(yr) | ||||
|
||||
Core-collapse SNRs | ||||
|
||||
J0536−6916 | SNR 1987A | 28 | Historical | Maggi et al. (2012b) |
J0540−6920 | B0540−693 | ~1600 | Pulsar | Kaaret et al. (2001) |
J0525−6938 | N132D | ~3150 | Ejecta, morphology | Borkowski et al. (2007) |
J0535−6602 | N63A | 2000−5000 | Ejecta, Fe K | Warren et al. (2003) |
J0536−6913 | − | 2200−4900 | Ejecta | Kavanagh et al. (2015a) |
J0505−6802 | N23 | ~4600 | Ejecta, CCO, morphology | Hughes et al. (2006) |
J0526−6605 | N49 | ~4800 | Ejecta, SGR, Fe K | Park et al. (2012) |
J0537−6910 | N157B | ~5000 c | PWN | Chen et al. (2006) |
J0525−6559 | N49B | ~10000 | Ejecta, morphology | Park et al. (2003b) |
J0536−6735 | DEM L241 | > 104 c | HMXB | Seward et al. (2012) |
J0453−6829 | B0453−685 | 12 000−1 5000 | PWN, morphology | Haberl et al. (2012a) |
J0531−7100 | N206 | ~25 000 | PWN candidate, morphology | Williams et al. (2005) |
|
||||
Type Ia SNRs | ||||
|
||||
J0509−6731 | B0509−675 | 400±120 | Light echo, ejecta | Rest et al. (2008) |
Fe K, morphology | ||||
|
||||
J0509−6844 | N103B | 860 | Ejecta, Fe K | Hughes et al. (1995) |
J0519−6902 | B0519−690 | 600 ± 200 | Ejecta, Fe K, morphology | Hughes et al. (1995) |
J0505−6753 | DEM L71 | ~4700 | Ejecta. Fe K, morphology | Hughes et al. (1998, 2003) |
J0547−7025 | B0548−704 | ~7100 | Ejecta | Hendrick et al. (2003), this work |
J0534−6955 | B0534−699 | ~10000 | Ejecta, morphology | Hendrick et al. (2003) |
J0534−7033 | DEM L238 | ~13500 | Ejecta | Borkowski et al. (2006) |
J0536−7039 | DEM L249 | ~15000 c | Ejecta | Borkowski et al. (2006) |
J0506−7026 | [HP99] 1139 | 17 000−21 000 | Ejecta | Kavanagh et al. (in prep.), this work |
J0508−6902 | [HP99] 791 | 20 000−25 000 | Ejecta | Bozzetto et al. (2014) |
J0527−7104 | [HP99] 1234 | ~25 000 | Ejecta | Kavanagh et al. (2013), this work |
J0547−6941 | DEM L316A | ~27 000c | Ejecta | Williams & Chu (2005) |
J0511−6759 | − | ≳ 20 000 c | Ejecta | Maggi et al. (2014) |
J0508−6830 | − | ≳ 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).
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.
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