Table 1
Observed properties of outbursting intermediate polars.
Name | P orb | Ωspin | Duration | τ rec | Comments | Refs. |
(h) | (mHz) | (day) | ||||
|
||||||
V455 And | 1.35 | 92.9 | 30 days | WZ Sge type superoutburst | 1 | |
CC Scl | 1.40 | 16.1 | 9 (SO) | SU UMa type | 2 | |
HT Cam | 1.43 | 12.2 | 1−2 | 3 | ||
DW Cnc | 1.44 | 2.71 | 2−3 | 4 | ||
EX Hya | 1.64 | 1.56 | 2−3 | 1.5 yr | 5 | |
V1223 Sgr | 3.36 | 8.43 | 0.25−1 | 6 | ||
YY Dra (=DO Dra) | 3.96 | 11.9 | 3−5 | 1 yr | 7 | |
TV Col | 5.49 | 3.29 | 0.25 | 8, 9 | ||
XY Ari | 6.61 | 30.5 | 5 | 10 | ||
CXOGBS J174954.5−294335 | 8.61 | 12.5 | > 0.25 | 11 | ||
GK Per | 47.9 | 17.9 | 60 | 2−3 yr | historical nova | 12 |
Reference. (1) Nogami et al. (2009); (2) Kato et al. (2015); (3) Ishioka et al. (2002); (4) Crawford et al. (2008); (5) Hellier et al. (2000); (6) van Amerongen & van Paradijs (1989); (7) Andronov et al. (2008); (8) Szkody & Mateo (1984); (9) Hudec et al. (2005); (10) Hellier et al. (1997); (11) Johnson et al. (2017); (12) Šimon (2015).
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