New low-mass members of the Octans stellar association and an updated 30-40 Myr lithium age

Monthly Notices of the Royal Astronomical Society(2015)

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摘要
The Octans association is one of several young stellar moving groups recently discovered in the Solar neighbourhood and hence a valuable laboratory for studies of stellar, circumstellar disc and planetary evolution. However, a lack of low-mass members or any members with trigonometric parallaxes means the age, distance and space motion of the group are poorly constrained. To better determine its m...
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关键词
stars: kinematics and dynamics,stars: low-mass,stars: pre-main-sequence,open clusters and associations: individual: Octans
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