Three new high-mass X-ray binaries in the Large Magellanic Cloud

Open Access

Table 2.

Optical counterparts of XMMU J045315.1−693242, XMMU J045736.9−692727, and RX J0524.2−6620.

Source	V ^(a)	Q (^a,^b)	2MASS	J	H	K_s	RA	Dec	D ^(d)
name							(J2000) ^(c)
	(mag)	(mag)		(mag)	(mag)	(mag)	(h m s)	(° ′ ″)	(″)
J0453	15.49	−0.85	04531503 − 6932416	15.51	15.19	15.27	04 53 15.05	−69 32 41.5	0.97
J0457	14.22	−1.33	04573695 − 6927275	13.50	13.38	13.18	04 57 36.95	−69 27 27.5	0.39
J0524	14.87	−0.94	05241180 − 6620512	14.70	14.69	14.59	05 24 11.81	−66 20 51.1	0.37

Notes.

^(a)

Magnitudes and colours from Zaritsky et al. (2004).

^(b)

Reddening-free parameter Q = U − B − 0.72(B − V). For the distribution of the Q parameter of BeXRBs in the SMC see Haberl & Sturm (2016).

^(c)

Position of the optical counterpart from Gaia EDR3 (see Gaia Collaboration 2021, 2016).

^(d)

Angular distance between XMM-Newton and Gaia position.

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.