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利用BATC和SDSS数据研究银河系恒星金属丰度分布 Abstract Metallicity,animportantparameterofastar,hassignificanteffectsonitsphysicalandchemicalproperties.Inthisstudy,weinvestigatethemetallicitydistributionofstarsintheMilkyWayusingthedatafromtheBaryonOscillationSpectroscopicSurvey(BOSS)oftheSloanDigitalSkySurvey(SDSS)andtheBeijing-Arizona-Taiwan-Connecticut(BATC)Multi-ColorSkySurvey.Throughspectroscopicmeasurementsandphotometricobservations,weobtainthemetallicitydistributionofstarsinseveralGalacticregions.Ourresultsshowthatthemetallicitydistributionvariesacrossthedifferentregions,withthehighestmetallicityintheGalacticplaneandthelowestintheGalactichalo.OurstudyprovidesimportantinsightsintothechemicalevolutionoftheMilkyWay. Introduction Metallicity,definedastheabundanceofelementsheavierthanheliuminastar,isafundamentalparameterthatdeterminesitsphysicalandchemicalproperties.Themetallicityofastaraffectsitsluminosity,temperature,andspectralcharacteristics.ThemetallicitydistributionofstarsintheMilkyWayprovidesimportantinformationaboutthechemicalevolutionoftheGalaxy,whichisakeyprocessintheformationandevolutionofgalaxies. SeveralstudieshaveinvestigatedthemetallicitydistributionofstarsintheMilkyWayusingvariousmethods,suchasspectroscopicmeasurementsandphotometricobservations.TheBaryonOscillationSpectroscopicSurvey(BOSS)oftheSloanDigitalSkySurvey(SDSS)hasprovidedspectroscopicmeasurementsofmillionsofstarsintheMilkyWay.TheBeijing-Arizona-Taiwan-Connecticut(BATC)Multi-ColorSkySurveyhasconductedphotometricobservationsoftheMilkyWayinmultiplewavebands,providingadditionalinformationonstellarpropertiessuchasmetallicity. Inthisstudy,weusethedatafromtheBOSSandBATCsurveystoinvestigatethemetallicitydistributionofstarsinseveralGalacticregions,includingtheGalacticplane,disk,andhalo.WeaimtoprovideacomprehensiveunderstandingofthemetallicitydistributionintheMilkyWayanditsimplicationsforthechemicalevolutionoftheGalaxy. DataandMethods WeusethedatafromtheBOSSandBATCsurveystoobtainthemetallicitydistributionofstarsintheMi