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NASA NTRS ยท 19720004115

Comments on an association in Vela

Abstract

Evidence for an association near the Vela pulsar rests on the H-R diagram. Definite bunching occurs around the mean line. However this evidence is not supported by correlation of proper motions in the region. If the Vela pulsar is a member of this association, a rather large mass is implied, about 10 solar masses.

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BibTeXRIS

Straka, W. C.. 1971-09-01. Comments on an association in Vela. https://ntrs.nasa.gov/citations/19720004115

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