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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.

(a)

for d = 5 kpc;

(b)

for d = 4 − 5 kpc, Gaia geometric distance 4.8 kpc (Bailer-Jones et al. 2021);

(c)

for d = 1 − 5 kpc;

(d)

also a hard bremmstahlung component detected;

(e)

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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