Four new X-ray-selected supernova remnants in the Large Magellanic Cloud

P. Maggi; F. Haberl; P. J. Kavanagh; S. D. Points; J. Dickel; L. M. Bozzetto; M. Sasaki; Y.-H. Chu; R. A. Gruendl; M. D. Filipović; W. Pietsch

doi:10.1051/0004-6361/201322820

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Volume 561 (January 2014)

A&A, 561 (2014) A76

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Table 1

XMM-Newton observations log, position, and size of the remnants.

MCSNR	Observation	Exposure time (ks)^a		Position of the remnant (J2000)		X-ray radius^b	Off-axis
	ID	pn	MOS1/2	RA	Dec	(arcmin)	angle^c

A: J0508−6830	0690742401	26.0	27.2	05^h08^m49.5^s	−68°30^m41^s	1.15( ± 0.10) × 0.90( ± 0.10)	10.9
B: J0511−6759	0690742201	25.1	28.9	05^h11^m10.7^s	−67°59^m07^s	0.93 ± 0.09	7.9
C: J0514−6840	0690742601	27.3	28.0	05^h14^m15.5^s	−68°40^m14^s	1.83 ± 0.12	10.0
C: J0514−6840	0690742701	29.5	33.6	05^h14^m15.5^s	−68°40^m14^s	1.83 ± 0.12	13.4
D: J0517−6759	0690741101	24.6	26.2	05^h17^m10.2^s	−67°59^m03^s	2.7( ± 0.1) × 1.8( ± 0.1)	4.1

Notes.

^(a)

Exposure times after removal of high background intervals.

^(b)

See Sect. 5.1 for details on the size of each remnant, or size at other wavelengths.

^(c)

Angle in arcmin between the aiming point of the observations and the centre of the X-ray source (as defined in Sect. 5.1).

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