Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-13T04:41:09.864Z Has data issue: false hasContentIssue false

A large high velocity cloud at lII = 41°, bII = −15°

Published online by Cambridge University Press:  14 August 2015

J. H. Oort*
Affiliation:
Leiden Observatory

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In a study made by Miss Gail Smith at Leiden a cloud was found with a rather exceptional velocity and a large velocity spread. The cloud is elongated, with a ratio of length to breadth of about 3 : 1. Its length is about 10°. The average velocity relative to the local standard of rest is +90 km/sec; the width of the profiles is considerable, corresponding to a halfwidth of about 30 km/sec. The mass can be estimated only if we know the distance. Taking 200 pc as a reasonable estimate of the minimum distance of the cloud the minimum mass is about 200 solar masses. The computed mass varies as the square of the distance.

Type
Section 1: The Galaxy
Copyright
Copyright © Australian Academy of Science 1964