Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-30T01:49:14.407Z Has data issue: false hasContentIssue false

The 06.5 IIIf star BD + 60°2522 and its interaction with the surrounding interstellar medium

Published online by Cambridge University Press:  04 August 2017

C. Chavarrîa-K.
Affiliation:
Landessternwarte Königstuhl D-6900 Heidelberg Germany
C. Jäger
Affiliation:
Landessternwarte Königstuhl D-6900 Heidelberg Germany
C. Leitherer
Affiliation:
Landessternwarte Königstuhl D-6900 Heidelberg Germany

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.

The luminous O-type star BD +60°2522 is embedded in the extended H II region S 162. Part of S 162 is NGC 7635, the striking spherically symmetric bubble nebula surrounding BD +60°2522. This star itself is unique in that it is the only known O star apparently associated with warm dust.

Type
Mass Loss from Hot Stars
Copyright
Copyright © Reidel 1987