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VLBI Observations of Water Masers in the Circumstellar Envelope of IRC$ +$60169

机译:VLBI IRC $ + $ 60169环绕星际中的水质观测

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WatermasersaroundanAGBstar,IRC$$+$$60169,wereobservedatfourepochsusingtheJapaneseVLBInetworks.Thedistributionofthemaserfeaturesislimitedinathick-shellregion,whichhasinnerandouterexpansionvelocitiesof$$7,mathrm{km},mathrm{s}^{-1}$$and$$14,mathrm{km},mathrm{s}^{-1}$$atradiiof25a€‰masand120a€‰mas,respectively.Thedistributionofthered-shiftedfeaturesexhibitsaring-likestructure,thediameterofwhichis30a€‰mas,andcorrespondstotheinnerradiusofthemasershell.Thisimpliesthatdensegasaroundthestarobscuresred-shiftedemission.Althoughapositiona€“radialvelocitydiagramforthemaserfeaturesisconsistentwithasphericalshellmodel,therelativepropermotionsdonotindicateanexpansionmotionoftheshell.Aremarkablepropertyhasbeenfoundthatisapossibleperiodicchangeofthealignmentpatternofwatermaserspots.
机译:使用日本VLBI网络在大约四个时期观察到一个AGBstar水星,IRC $$ + $ 60169,其特征分布限制在厚壳区域内,该区域的内部和外部扩展速度分别为$ 7,mathrm {km},mathrm {s} ^ {-1} $ {和$ 14} -1} $$ atradiiof25a€‰masand120a€‰MAS,respectively.Thedistributionofthered-shiftedfeaturesexhibitsaring-likestructure,thediameterofwhichis30a€‰MAS,andcorrespondstotheinnerradiusofthemasershell.Thisimpliesthatdensegasaroundthestarobscuresred-shiftedemission.Althoughapositiona€“radialvelocitydiagramforthemaserfeaturesisconsistentwithasphericalshellmodel,therelativepropermotionsdonotindicateanexpansionmotionoftheshell.Aremarkablepropertyhasbeenfoundthatisapossibleperiodicchangeofthealignmentpatternofwatermaserspots。

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