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时间:2019-06-19
《ASTROMETRIC-SPECTROSCOPIC DETERMINATION OF THE ABSOLUTE MASSES英文资料》由会员上传分享,免费在线阅读,更多相关内容在学术论文-天天文库。
1、TheAstronomicalJournal,133:2684Y2695,2007June#2007.TheAmericanAstronomicalSociety.Allrightsreserved.PrintedinU.S.A.ASTROMETRIC-SPECTROSCOPICDETERMINATIONOFTHEABSOLUTEMASSESOFTHEHgMnBINARYSTARHERCULISGuillermoTorresHarvard-SmithsonianCenterforAstrophysics,Cambridge,MA02138,USA;gtorres@cfa.harv
2、ard.eduReceived2006December1;accepted2007February27ABSTRACTThemercury-manganesestarHerisawell-knownspectroscopicbinarythathasbeenthesubjectofarecentstudybyZavalaandcoworkersinwhichtheyresolvedthecompanionusinglong-baselineinterferometry.Thetotalmassofthebinaryisnowfairlywellestablished,butthe
3、combinationofspectroscopywithastrometryhasnotresultedinindividualmassesconsistentwiththespectraltypesofthecomponents.ThemotionofthecenteroflightofHerwasclearlydetectedbytheHipparcossatellite.HerewemakeuseoftheHipparcosintermediatedata(abscissaresiduals)andshowthatbycombiningtheminanoptimalfas
4、hionwiththeinterferometrytheindi-vidualmassescanbeobtainedreliablyusingonlyastrometry.Wereexamineandthenincorporateexistingradialvelocitymeasurementsintotheorbitalsolution,obtainingimprovedmassesof3:050:24and1:6140:066Mthatareconsistentwiththetheoreticalmass-luminosityrelationfromrecentstell
5、arevolutionmodels.Thesemassdeterminationsprovideimportantinformationfortheunderstandingofthenatureofthispeculiarclassofstars.Keywords:binaries:generalbinaries:spectroscopicmethods:dataanalysisstars:chemicallypeculiarstars:fundamentalparametersstars:individual(Herculis)1.INTRODUCTION2003;Dwore
6、tsky&Budaj2000;Leushin1995andreferencestherein).InarecentpaperZavalaetal.(2007)reportedinterferometricWewerepuzzledbythisapparentinconsistencybetweentheobservationsofthemercury-manganesestarHer[HD145389,hmsseeminglypreciseradialvelocitiesandtheastrometry,andweHR6023,HIP79101,J2000:0¼160846:18
7、,J2000:0¼000wonderedwhetherothervelocitymeasurementsavailableintheþ445605:7,spectraltypeB9:p(HgMn),V¼4:22],whichisliteraturemightclarifythesituation.Inaddition,Herwasob-abinarystar.Thisobjectbelongstoaclassofpeculiarnon-servedintheco
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