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Table 1.

Currently known AM CVn stars ordered by increasing period, either the orbital period (most reliably determined from spectroscopic observations) or the superhump period (sh) which is typically within a few percent longer than the orbital period.

Source Period Outbursts? Mag. Range Reference Parallax σ Distance σ
(mins) (filter) (mas) (mas) (pc) (pc)
HM Cnc 5.4 21.1 1
V407 Vul 9.5 19.9 (V) 2 0.095 0.327 1786 667
ES Cet 10.4 16.5–16.8 3 0.596 0.108 1584 291
SDSS J1351-0643 15.7 18.6 43 0.596 0.313 1317 531
AM CVn 17.1 14.2 4 3.351 0.045 299.1 4.4
SDSS J1908+3940 18.1 16.1 5, 6 0.954 0.046 1044 51
HP Lib 18.4 13.6–13.7 7 3.62 0.05 276 4
PTF1 J1919+4815 22.5 18.2–21.8 8 0.550 0.327 1339 555
CX361 22.9 17.6 9 1.016 0.146 971 156
ASASSN-14cc 22.5 (sh) 16.0–20.0 (V) 10 0.975 0.098 1019 108
CR Boo 24.5 13.8–17.0 11
KL Dra 25.0 16.0–19.6 12 1.035 0.149 956 153
PTF1 J2219+3135 26.1 (p) 16.2–20.6 14
V803 Cen 26.6 12.8–17.0 13, 14
PTF1 J0719+4858 26.8 15.8–19.4 15 1.144 0.301 861 304
ASASSN-15kf 27.7 (sh) 15.0 (V) –19.4 (B) 16, 17
YZ LMi (SDSS J0926+3624) 28.3 16.6–19.6 18 1.824 0.549 577 324
CP Eri 28.4 16.2–20.2 19 0.684 0.941 964 615
SDSS J1043+5632 28.5:(p) 17.0–20.3 14 0.830 0.668 979 575
CRTS J0910-2008 29.7 (sh) 14.0–20.4 (g) 45 0.695 0.477 1113 561
PTF1 J0943+1029 30.4 16.9 (R)–20.7 (g) 20
CRTS J0105+1903 31.6 16.3-19.6 21, 22 1.382 0.457 734 374
PTF1 J1632+3511 32.7 (p) 17.9–23.0 20
CRTS J0744+3254 33: (p) 17.4–21.1 14
V406 Hya 33.8 14.5–19.7 23 2.391 1.050 504 493
PTF1J0435+0029 34.3 18.4 (R) – 22.3 (g) 20
SDSS J1730+5545 35.2 18.5 (V) –20.1 14, 24a 1.061 0.382 911 420
V558 Vir (2QZ J1427-0123) 36.6 (sh) 15.0–20.5 25 1.911 1.425 677 595
SDSS J1240-0159 37.4 16.8–19.8 27 1.857 0.611 577 365
NSV1440 37.5 (sh) 12.4(V) – 17.9(G) 45 2.971 0.142 337 17
V744 And (SDSS J0129+3842) 37.6 14.5–19.8 14, 26, 29 2.066 0.529 508 239
SDSS J1721+2733 38.1 16.0–20.1 14, 31 0.798 0.665 995 578
ASASSN-14mv 41: (sh) 11.8 (V) – 18.1 (V) 16, 17, 44 4.069 0.119 247 7
ASASSN-14ei 43: (sh) 11.9–17.6 (B) 17, 33 3.92 0.045 255 4
SDSS J1525+3600 44.3 20.2 31 1.928 0.276 524 90
SDSS J0804+1616 44.5 17.8–19.0 28, 30 1.203 0.210 828 173
SDSS J1411+4812 46.0 12.4–19.7 29, 30, 48 2.361 0.305 429 65
GP Com 46.6 15.9–16.3 32 13.731 0.060 73.0 0.4
CRTS J0450-0931 47.3 (sh) 14.8–20.5 34
SDSS J0902+3819 48.3 13.8 (V) – 20.2 (g) 15, 31, 35 2.519 0.936 461 435
Gaia14aae 49.7 13.6 (V) – 18.7 (g) 36, 49 3.871 0.155 259 11
ASASSN-17fp 51.0 (sh) 15.7–20+ 37
SDSS J1208+3550 53.0 18.9–19.4 30, 38, 39 5.005 0.416 202 18
SDSS J1642+1934 54.2 20.3 31, 39 0.621 0.730 1044 604
SDSS J1552+3201 56.3 20.2–20.6 30, 41 2.395 0.609 443 227
SDSS J1137+4054 59.6: 19.0 24b 4.838 0.310 209 14
V396 Hya 65.1 17.6 42 10.694 0.148 93.6 1.4
SDSS J1319+5915 65.6 19.1 40,47 4.894 0.240 205 10
PU Aqr (SDSS J2047+0008) ? 17.0–24 38
CRTS J0844-0128 ? 17.4–20.3 14 0.395 0.341 1474 597
PTF1 J0857+0729 ? 18.6–21.8 14
SDSS J1505+0659 ? 19.1 24b 6.299 0.453 160 12
PTF1 J1523+1845 ? 17.6–23.5 14
ASASSN-14fv ? 14.6 (V) – 20.5 (B) 41
Gaia16all ? 16.2 – 20.6(G) 46 0.760 0.859 956 605
SDSS J0807+4852 ? 19.5(V)–20.4(g) 50 0.055 2.42 883 648

Notes. (p) implies the predicted orbital period based on the outburst properties (Levitan et al. 2015). ✓ or ✗ indicates whether the source has been seen in outburst. The references and full coordinates are given in Appendix A.2.

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