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...ью период — светимость]]<ref name="aavso"/>. Все известные переменные типа SX Феникса в шаровых скоплениях являются [[Г ...

| variable = [[SX Phoenicis variable|SX Phe]](?)<ref name=Samus_et_al_2017/> ...nicis]],<ref name=Andreasen_1983/> and by 1995 it was classified as a [[SX Phoenicis variable]] and a possible [[Stellar halo|halo]] object. However, [[Eric G. ...

| variable = [[SX Phoenicis variable|SX Phe]]<ref name=Xue_Niu_2020/><ref name=Samus_et_al_2017/> ...nstellation)|Pegasus]]. It is a well-studied<ref name=Fu_et_al_2009/> [[SX Phoenicis variable]] star with a brightness that ranges from an [[apparent visual mag ...

...ohen2012/> One last sub-class are the pre-main sequence (PMS) Delta Scuti variables. ...nt star|giant]] or [[main sequence]] stars. The high-amplitude Delta Scuti variables are also called '''AI Velorum stars''', after the prototype [[AI Velorum]]. ...

...idly oscillating Ap star]]s (roAps) near the [[main sequence]]; [[RR Lyrae variables]] where it intersects the [[horizontal branch]]; and the [[Cepheid variable ...scillating Ap star|roAp stars]] and the [[Delta Scuti variable|Delta Scuti variables]].<ref name="Warner1992">{{cite book | editor = Brian Warner | date = 1992 ...

...irst5 = Corinne | title = Driving the Gravity-Mode Pulsations in γ Doradus Variables | date = 10 October 2000 | journal = The Astrophysical Journal Letters | vo === Cepheid variables === ...

| title=The pulsations of AI Velorum, SX Phoenicis and RR Lyrae [[Category:Delta Scuti variables]] ...

...f merged stars may be measurably different from those of typical pulsating variables of similar mass and luminosity. However, the measurement of pulsations is v * {{annotated link|SX Phoenicis variable}} ...