Table 1.
AMXPs discovered so far and their main properties.
| Source | Porb | Ps | fX | M2, min | Year of | Ref. |
|---|---|---|---|---|---|---|
| (h) | (ms) | (M⊙) | (M⊙) | discovery | ||
| Aql X-1 | 18.95 | 1.7 | 1.4 × 10−2xs | 0.56 | 2008 | [6], [14] |
| IGR J18245–2452 | 11.03 | 3.9 | 2.3 × 10−3 | 0.17 | 2013 | [17] |
| Swift J1749.4–2807 | 8.82 | 1.9 | 5.5 × 10−2 | 0.59 | 2010 | [3] |
| IGR J17591–2342 | 8.80 | 1.9 | 1.5 × 10−2 | 0.42 | 2018 | [23] |
| SAX J1748.9–2021 | 8.77 | 2.3 | 4.8 × 10−3 | 0.10 | 2008 | [1] |
| XSS J12270–4859 | 6.91 | 1.7 | 3.9 × 10−3 | 0.27 | 2015 | [18] |
| PSR J1023+0038 | 4.75 | 1.7 | 1.1 × 10−3 | 0.20 | 2009 | [4], [7] |
| XTE J1814–338 | 4.27 | 3.2 | 2.0 × 10−3 | 0.17 | 2003 | [13] |
| IGR J17498–2921 | 3.84 | 2.5 | 2.0 × 10−3 | 0.17 | 2011 | [16] |
| IGR J17511–3057 | 3.47 | 4.1 | 1.1 × 10−3 | 0.13 | 2010 | [15] |
| IGR J00291+5934 | 2.46 | 1.7 | 2.8 × 10−3 | 0.039 | 2005 | [9] |
| SAX J1808.4–3658 | 2.01 | 2.5 | 3.8 × 10−5 | 0.043 | 1998 | [25] |
| IGR J1737.9–3747 | 1.88 | 2.1 | 8.5 × 10−5 | 0.056 | 2018 | [21] |
| HETE J1900.1–2455 | 1.39 | 2.7 | 2.0 × 10−6 | 0.016 | 2006 | [10] |
| NGC 6440 X-2 | 0.95 | 4.8 | 1.6 × 10−7 | 0.00067 | 2010 | [2] |
| Swift J1756.9–2508 | 0.91 | 5.5 | 1.6 × 10−7 | 0.0070 | 2007 | [11], [22] |
| IGR J16597–3704 | 0.77 | 9.5 | 1.2 × 10−7 | 0.0060 | 2017 | [20] |
| MAXI J0911–655 | 0.74 | 2.9 | 6.2 × 10−6 | 0.024 | 2016 | [19] |
| XTE J0929–314 | 0.73 | 5.4 | 2.9 × 10−7 | 0.0083 | 2002 | [8] |
| XTE J1751–305 | 0.71 | 2.3 | 1.3 × 10−6 | 0.014 | 2002 | [12] |
| XTE J1807–294 | 0.67 | 5.3 | 1.5 × 10−7 | 0.0066 | 2003 | [5] |
| IGR J17062–6143 | 0.64 | 6.1 | 9.1 × 10−8 | 0.00060 | 2017 | [24] |
Notes. In the table Porb is the orbital period, Ps is the spin period of the pulsar, fX is the mass function, and M2, min is the minimum mass for the companion, evaluated from fX for an inclination of 90°.
References. [1] = Altamirano et al. (2008), [2] = Altamirano et al. (2010a), [3] = Altamirano et al. (2011), [4] = Archibald et al. (2009), [5] = Campana et al. (2003), [6] = Casella et al. (2008), [7] = Coti Zelati et al. (2014), [8] = Galloway et al. (2002), [9] = Galloway et al. (2005a), [10] = Kaaret et al. (2006), [11] = Krimm et al. (2007), [12] = Markwardt et al. (2002b), [13] = Markwardt et al. (2003), [14] = Mata Sánchez et al. (2017), [15] = Papitto et al. (2010), [16] = Papitto et al. (2011a), [17] = Papitto et al. (2013a), [18] = Roy et al. (2015), [19] = Sanna et al. (2017a), [20] = Sanna et al. (2018b), [21] = Sanna et al. (2018c), [22] = Sanna et al. (2018d), [23] = Sanna et al. (2018a), [24] = Strohmayer et al. (2018b), [25] = Wijnands & van der Klis (1998).
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