Table 4.
Properties of DD ultra-compact binaries.
Source | Orbital period | kT | LX | log(fX/fopt) | g′−r′ | References |
---|---|---|---|---|---|---|
[min] | [eV] | [erg s−1] | ||||
HM Cnc | 5.4 | 65 | (a)4.5 × 1034 | (e)2.3 (2.4) | −0.44 | 1, 2, 7 |
V407 Vul | 9.5 | 43 | (b)5 × 1035–4 × 1036 | (e)1.6 (3.5) | 0.99 | 3, 4, 7, 8 |
3XMM J051034.6−682640 | 23.6 | 69 | (a)5 × 1032 | (e)1.1 (1.2) | −0.03 | 5, 6 |
eRASSU J060839.5−704014 | 6.2 | (d)110 | (c)6 × 1031–1.5 × 1033 | (e)1.6 (1.9) | 0.25 | This work |
Notes.
for d = 4 − 5 kpc, Gaia geometric distance 4.8 kpc (Bailer-Jones et al. 2021);
computed with the information of the mean g′ magnitude and maximum observed FX (un-absorbed and reddening-corrected). The g′−r′ colours were obtained after reddening correction. The luminosities were corrected for absorption.
References. (1) Israel et al. (2003); (2) Schlegel (2005); (3) Haberl & Motch (1995); (4) Cropper et al. (1998); (5) Ramsay et al. (2018); (6) Haberl et al. (2017); (7) Barros et al. (2007); (8) Ramsay (2008).
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