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Orbital Period Studies of Three Algols: TW And, RW Leo, and AY Vul

机译:TW And,RW Leo和AY Vul三个算法的轨道周期研究

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ThechangesintheorbitalperiodsofthreeEA-typeeclipsingbinaries,TWAnd,RWLeo,andAYVul,arediscussedbasedonananalysisoftheir$$O-C$$curves.ForRWLeo,itsorbitalperiodwasrevisedand,assumingacyclicoscillationintheorbitalperiod,aperiodof38.4a€‰yrwasdetermined.Fortheothertwosystems,TWAndandAYVul,their$$O-C$$diagramsshowcomplexvariations.Undertheassumptionofperiodicoscillation,cyclicchangeswithperiodsof56.4and78.6a€‰yrwerediscoveredtosuperimposeonupwardparabolicchanges,indicatingasecularperiodincrease.Thesecularperiodincreasesforthetwobinarysystemsindicatethattheyareonanactivephaseofmasstransfer.Assumingtheoscillationsintheperiodstobecausedbylight-timeeffectsduetothepresenceofa€?thirdbodiesa€?rotatingaroundthesebinarystars,theorbitalparametersofthethirdbodiesweredetermined.ForRWLeo,itispossibletodetectanadditionalthirdbodyphotometricallyandspectroscopically.However,fortheothertwosystems,TWAndandAYVul,itislesslikelytoseeadditionalbodies,unlesstheorbitalinclinationisverysmall(i.e.,$$i^{prime}30^{circ}$$).Newphotometricandspectroscopicobservationsandacarefulanalysisofthosedataareneededtocheckthepresenceofthirdbodies.
机译:ThechangesintheorbitalperiodsofthreeEA-typeeclipsingbinaries,TWAnd,RWLeo,andAYVul,arediscussedbasedonananalysisoftheir $$ OC $$ curves.ForRWLeo,itsorbitalperiodwasrevisedand,assumingacyclicoscillationintheorbitalperiod,aperiodof38.4a€‰yrwasdetermined.Fortheothertwosystems,TWAndandAYVul,他们$$ OC $$ diagramsshowcomplexvariations.Undertheassumptionofperiodicoscillation,cyclicchangeswithperiodsof56.4and78.6a €‰yrwerediscoveredtosuperimposeonupwardparabolicchanges,indicatingasecularperiodincrease.Thesecularperiodincreasesforthetwobinarysystemsindicatethattheyareonanactivephaseofmasstransfer.Assumingtheoscillationsintheperiodstobecausedbylight-timeeffectsduetothepresenceofa€thirdbodiesa€rotatingaroundthesebinarystars,theorbitalparametersofthethirdbodiesweredetermined.ForRWLeo,itispossibletodetectanadditionalthirdbodyphotometricallyandspectroscopically.However,fortheothertwosystems,TWAndandAYVul,itislesslikelytoseeadditionalbodies,unlesstheorbitalinclinationisverysmall(即,$$ I ^ {}素LT;?30 ^ {CI rc} $$)。新的光度法和分光镜观察以及对这些数据的仔细分析,有助于检查第三主体的存在。

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