High-mass X-ray binaries as members of open clusters

Open Access

Table 1.

High-mass X-ray binaries and candidates associated with OCs.

HMXB	Class	Secondary	OC	Astrometric membership (Hunt & Reffert 2024)	OC Age
		spectral type		probability	(Myr)
IGR J16465-4507	sgHMXB	B0.5-B1 Ib	CWNU 2672	1.0	1.2 – $18_{- 13}^{+ 29}$ $Mathematical equation: $ 18^{+29}_{-13} $$
SGR 0755-2933	BeXRB	B0Ve	HSC 1981	1.0	$20_{- 3}^{+ 5}$ $Mathematical equation: $ 20^{+5}_{-3} $$
HD 119682	γ Cas	B0Ve	NGC 5281	0.87	∼40 – 100
NGC 6649 9	γ Cas	B0Ve	NGC 6649	1.0	∼28 – 70

Notes. Column 1: HMXB designation. Column 2: Classification (sgHMXB = supergiant HMXB, BeXRB = Be X-ray binary, γ Cas = gamma Cassiopeiae analog). Column 3: Spectral type of the secondary star. Column 4: OC designation. Column 5: OC membership probability. Column 6: OC age estimates from the literature.

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.