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Formation scenarios for the young stellar associations between galactic longitudes l $\mathsf{= 280\degr{-}360\degr}$

ASTRONOMY & ASTROPHYSICS, no. 3 (2003): 913-926

Cited: 109|Views24

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stars : formationstars : pre-main sequencestars : early-typestars : kinematicsstars : Hertzsprung-Russell (HR) and C-M diagramsMore(1+)

Abstract

We investigate the spatial distribution, the space velocities and age distribution of the pre-main sequence (PMS) stars belonging to Ophiuchus, Lupus and Chamaeleon star-forming regions (SFRs), and of the young early-type star members of the Scorpius-Centaurus OB association. These young stellar associations extend over the galactic longi...More

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marilia j sartori

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j r d lepine

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w s dias

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