Subject |
is part of |
is an instance of |
has prototype |
is a kind of |
has definition |
SS Cygni star | | | | dwarf nova | A subclass of dwarf nova. SS Cyg is a double-lined, noneclipsing spectroscopic binary (sdBe, dG5) with an orbital period of 6h38m. Mean time between eruptions, 54 days. It may be a sporadic source of soft X-rays. |
SU Ursa Major | Milky Way | dwarf nova | | | |
U Geminorum star | | | U Geminorum | dwarf nova | A type of dwarf nova. All U Geminorum stars are binaries containing a white dwarf and a red dwarf with total masses of roughly 1-2 Msun and with periods of less than 12 hours (period of U Gem, 1.5 × 104 seconds). About 150 are known. |
VW Hydri | Milky Way | dwarf nova | | | |
Z Camelopardalis star | | | Z Camelopardalis | dwarf nova | A class of dwarf nova with standstills in their light curves. Z Cam itself is a semidetached binary (period 7h21m) consisting of a dG1 star and a hot white dwarf or a hot blue subdwarf which is probably degenerate. Mean time between eruptions, 20 days. Peak-to-peak amplitude, about 0.5 mag. |