Supernova remnants on the outskirts of the Large Magellanic Cloud

Open Access

Table A.1.

Best-fit values for the spectra of SNR J0614–7251 for the outer shell only and for the entire source using two components.


Shell	ISM

N_H [10²⁰ cm⁻²]	< 3.5
kT [keV]	$0 . 49_{- 0.12}^{+ 0.11}$ $0.49^{+0.11}_{-0.12}$
Fe [Z_⊙]	0.5^†
τ [×10¹⁰ s cm⁻³]	$1 . 28_{- 0.41}^{+ 0.87}$ $1.28^{+0.87}_{-0.41}$
EM [10⁵⁷ cm⁻³]	$1 . 50_{- 0.27}^{+ 0.44}$ $1.50^{+0.44}_{-0.27}$
d.o.f.	116
χ_red	1.08


Entire SNR	ISM	ejecta


N_H [10²⁰ cm⁻²]	0.0^†	0.0^†
kT [keV]	0.49^†	$0 . 47_{- 0.03}^{+ 0.09}$ $0.47^{+0.09}_{-0.03}$
Fe [Z_⊙]	0.5^†	> 0.75
τ [×10¹⁰ s cm⁻³]	1.28^†	> 4720
EM [10⁵⁷ cm⁻³]	$2 . 13_{- 0.18}^{+ 0.13}$ $2.13^{+0.13}_{-0.18}$	$0 . 41_{- 0.41}^{+ 1.05}$ $0.41^{+1.05}_{-0.41}$
d.o.f.	185
χ_red	1.21

^†These value were fixed.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.