The current state of disk wind observations in BHLMXBs through X-ray absorption lines in the iron band

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Volume 681 (January 2024)

A&A, 681 (2024) A49

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Table 2.

Details of accretion states with reports of absorption line detection in both our work and the literature.

Source	Accretion states with absorption lines reported
	This work	Other works
	Iron band	Iron band	Other energies
4U 1543-47	X	soft⁽¹⁾	X
4U 1630-47	soft	soft ⁽²⁾	soft^X⁽³⁾
EXO 1846-031	X	hard⁽⁴⁾	X
GRO J1655-40	soft	soft ⁽⁵⁾	soft^X⁽⁶⁾
GRS 1716-249	X	X	hard^V⁽⁷⁾
GRS 1758-258	X	hard (8)	X
GRS 1915+105	soft, hard	soft:ϕ, γ, ρ, β⁽⁹⁾, θ⁽¹⁰⁾, κ⁽¹¹⁾, λ⁽¹²⁾, hard:χ⁽¹³⁾, obscured^( * ,15)	soft^X:ϕ⁽¹⁴⁾, obscured^( * ):hard^IR⁽¹⁶⁾
GX 339-4	X	X	soft^V⁽¹⁷⁾, hard^V⁽¹⁷⁾
H 1743-322	soft	soft ⁽¹⁸⁾	X
IGR J17091-3624	X	soft ⁽¹⁹⁾, hard^{( † ,20)}	hard^X⁽²¹⁾
IGR J17451-3022	soft	soft ⁽²²⁾	soft^X⁽²²⁾
MAXI J1305-704	X	soft^(23, 24), hard⁽²⁴⁾	soft^X^(23, 24), hard^X⁽²⁴⁾
MAXI J1348-630	X	soft⁽²⁵⁾, hard⁽²⁵⁾	hard^X⁽²⁶⁾, soft^IR⁽²⁷⁾, hard^V, IR⁽²⁷⁾
MAXI J1803-298	X	soft ^(28, 29)	hard^V⁽³⁰⁾
MAXI J1820+070	X	soft ⁽³¹⁾	soft^IR⁽³²⁾, hard^V, IR⁽³²⁾
Swift J1357.2-0933	X	X	hard^V^(33, 34)
Swift J1658.2-4242	X	hard⁽³⁵⁾	X
V404 Cyg	X	hard ⁽³⁶⁾	obscured^( * ): hard^X⁽³⁷⁾, hard^V⁽³⁸⁾
V4641 Sgr	X	X	obscured^( * ): hard^V⁽³⁹⁾
XTE J1652-453	X	hard^{( † ,40)}	X

Notes. The source names in bold indicate dippers. For “other” energies, X superscripts indicate softer X-ray detections, V indicates visible detections, and IR notes infrared detections. Accretion states are reported in italics for absorption lines embedded in reflection components. For all purposes, ^( † )indicates low-significance detections. ^( * )The observed HR value of the obscured state might not reflect the actual HR of the source. The list of reference papers is not exhaustive for objects with many wind detections.

References. (1) Prabhakar et al. (2023). (2) Kubota et al. (2007). (3) Trueba et al. (2019). (4) Wang et al. (2020). (5) Miller et al. (2006a). (6) Miller et al. (2008). (7) Cúneo et al. (2020). (8) Reynolds et al. (2018). (9) Neilsen & Lee (2009). (10) Ueda et al. (2010). (11) Liu et al. (2022). (12) Neilsen et al. (2018). (13) Lee et al. (2002). (14) Ueda et al. (2009). (15) Neilsen et al. (2020). (16) Sánchez-Sierras et al. (2023a). (17) Rahoui et al. (2014). (18) Miller et al. (2006b). (19) King et al. (2012). (20) Wang et al. (2018). (21) Gatuzz et al. (2020) (22) Jaisawal et al. (2015). (23) Miller et al. (2014). (24) Shidatsu et al. (2013). (25) Chakraborty et al. (2021). (26) Saha et al. (2021). (27) Panizo-Espinar et al. (2022). (28) Miller & Reynolds (2021). (29) Coughenour et al. (2023). (30) Mata Sánchez et al. (2022). (31) Fabian et al. (2021). (32) Muñoz-Darias et al. (2019). (33) Jiménez-Ibarra et al. (2019). (34) Charles et al. (2019). (35) Xu et al. (2018a). (36) Muñoz-Darias & Ponti (2022). (37) King et al. (2015). (38) Muñoz-Darias et al. (2016). (39) Muñoz-Darias et al. (2018). (40) Chiang et al. (2012).

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