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Age Sequence in Small Clusters Associated with Bright-Rimmed Clouds
[摘要] Bright-rimmedclouds(BRCs)foundinHIIregionsareprobablesitesoftriggeredstarformationduetocompressionbyionization/shockfronts,anditishypothesizedthatstarformationproceedsfromtheexcitingstar(s)sideoutwardoftheHIIregion(“small-scalesequentialstarformation”).Inordertoquantitativelytestthishypothesisweundertook$$BVI_mathrm{c}$$photometryoffourBRCaggregates.Theamountsofinterstellarextinctionandreddeningforeachstarwereestimatedbyusing$$JHK_mathrm{s}$$photometry.Wethenconstructedreddening-corrected$$V/V-I_mathrm{c}$$color-magnitudediagrams,wheretheageofeachstarwasderived.AllofthestarsturnedouttobeafewtenthstoafewMyrold.Althoughthescatterswerelargeandthenumbersofthesamplestarsaresmall,wefoundacleartrendthatthestarsinsideorintheimmediatevicinityofthebrightrimareyoungerthanthoseoutsideitinallfouraggregates,confirmingthehypothesisinquestion.
[发布日期]  [发布机构] 
[效力级别]  [学科分类] 天文学(综合)
[关键词] "open clusters and associations: general";"ISM: bubbles";"HII regions";"stars: formation";"stars: pre-main sequence" [时效性] 
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