Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-22T05:56:22.255Z Has data issue: false hasContentIssue false

The Globular Cluster NGC 6266

Published online by Cambridge University Press:  25 April 2016

S. C. B. Gascoigne
Affiliation:
Mount Stromlo Observatory, Australian National University, Canberra
V. Ford
Affiliation:
Mount Stromlo Observatory, Australian National University, Canberra

Extract

This cluster has two notable characteristics: it contains more than 80 variables, and relative to its NP half its SF half is covered by a cloud absorbing up to a magnitude in the blue. These properties make it an ideal object for determining the ratio Av/E of V absorption to colour excess—one simply compares mean colours and magnitudes of variables in the obscured part with those in the clear part.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1967

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)