Also called a flashing star. A type of variable star that increases in brightness irregularly and suddenly, then returns to its original brightness within a short time. It is thought to be caused by a mechanism similar to the solar flare. UV Ceti, RS Cana Venatici, etc. Source : Heibonsha Encyclopedia About MyPedia Information |
せん(閃)光星とも。変光星の一種で,不規則・突発的に明るさを増し,その後短時間のうちに元の明るさに戻るものをいう。太陽で生じるフレアと類似の機構によると考えられている。くじら座UV星,りょうけん座RS星など。
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