Table 2.
Characteristics of LMXBs with OIR winds and properties of the outflow.
(a) OIR wind detections | |||||||
---|---|---|---|---|---|---|---|
LMXB | Object | i (°) | P (h) | Wind features | Vel. (km s−1) (a) | Spectral range | References |
GX13+1 | NS | 60–80 | 589 | P-Cygni | ∼2400 | NIR | 1, 1b, 1c, 1d |
V404 Cyg | BH | 60–70 | 155.3 | P-Cygni | 1500–3000 | Optical | 2, 2b, 2c, 2d, 2e |
Broad wings | ∼3000 | ||||||
V4641 Sgr | BH | 60–70 | 67.6 | P-Cygni | 900–1600 | Optical | 3, 3b, 3c, 3d, 3e |
Broad wings | ∼3000 | ||||||
Swift J1357.2−0933 | BH | ≳80 | 2.8 | P-Cygni | 1600–4000 | Optical | 4, 4b, 4c |
MAXI J1820+070 | BH | 67–81 | 16.4 | P-Cygni | 1200–1800 | Optical | 5, 5b, 5c, 5d |
Broad wings | ∼1800 | Optical | |||||
Blueshifted abs. (b) | 1200–1800 | NIR | |||||
Swift J1858.6−0814 | NS | Dipping/eclipsing | 21.8 | P-Cygni | 1700–2400 | Optical | 6, 6b, 6c |
GRS1716-249 | BH | ? | ? | P-Cygni | ∼2000 | Optical | 7 |
Flat-top, asymmetries | − | ||||||
MAXI J1803–298 | BH | Dipping | 7–8 | P-Cygni | ∼1250 | Optical | 8, 8b, 8c |
MAXI J1348–630 | BH | Mid-to-low | ? | Broad wings | 1500–1700 | Optical, NIR | this work, 9 |
Blueshifted abs. | 500–900 | Optical, NIR | |||||
Flat-top, asymmetries | − | Optical, NIR | |||||
(b) Tentative OIR wind detections | |||||||
LMXB | Object | i (°) | P (h) | Wind features | Vel. (km s−1) (a) | Spectral range | References |
Sco X-1 | NS | < 40 | 18.9 | P-Cygni | ∼2600 | NIR | 1, 10, 10b, 10c |
GRO J1655–40 | BH | 67–70 | 62.9 | Flat-top, asymmetries | − | Optical | 11, 11b, 11c |
GX339–4 | BH | 37–78 | 42.2 | Broad wings | ? | NIR | 12, 12b |
Aql X-1 | NS | 23–53 | 18.7 | Broad wings | 800 | Optical | 13, 13b, 13c |
Notes.
References. (1) Bandyopadhyay et al. (1999); (1b) Iaria et al. (2014); (1c) Díaz Trigo et al. (2012); (1d) Homan et al. (2016); (2) Muñoz-Darias et al. (2016); (2b) Muñoz-Darias et al. (2017); (2c) Mata Sánchez et al. (2018); (2d) Casares et al. (1991); (2e) Khargharia et al. (2010); (3) Muñoz-Darias et al. (2018); (3b) Lindstrøm et al. (2005); (3c) Chaty et al. (2003); (3d) Orosz et al. (2001); (3e) Macdonald et al. (2014); (4) Jiménez-Ibarra et al. (2019); (4b) Mata-Sánchez et al. (2015a); (4c) Corral-Santana et al. (2013); (5) Muñoz-Darias et al. (2019); (5b) Sánchez-Sierras & Muñoz-Darias (2020); (5c) Torres et al. (2019); (5d) Torres et al. (2020); (6) Muñoz-Darias et al. (2020); (6b) Buisson et al. (2020); (6c) Buisson et al. (2021); (7) Cúneo et al. (2020b); (8) Mata Sánchez et al. (2022); (8b) Homan et al. (2021); (8c) Xu et al. (2021); (9) Carotenuto et al. (2022); (10) Fomalont et al. (2001); (10b) Gottlieb et al. (1975); (10c) Mata Sánchez et al. (2015b); (11) Soria et al. (2000); (11b) van der Hooft et al. (1998); (11c) Beer & Podsiadlowski (2002); (12) Rahoui et al. (2014); (12b) Heida et al. (2017); (13) Panizo-Espinar et al. (2021); (13b) Mata Sánchez et al. (2017); (13c) Chevalier & Ilovaisky (1991).
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