Hostname: page-component-848d4c4894-pjpqr Total loading time: 0 Render date: 2024-06-19T14:31:07.632Z Has data issue: false hasContentIssue false
  • English
  • Français

CO and CS Observations in the Eastern Part of W5

Published online by Cambridge University Press:  04 August 2017

S. Wramdemark ,
G. Lyngå  and
L.E.B. Johansson
S. Wramdemark
Affiliation:
Lund Observatory, S-221 00 Lund, Sweden
G. Lyngå
Affiliation:
Lund Observatory, S-221 00 Lund, Sweden
L.E.B. Johansson
Affiliation:
Onsala Space Observatory, S-430 34 Onsala, Sweden

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.

At galactic longitudes between 132 and 139 degrees and distances of 2 to 2.5 kpc, the galactic disk contains an unusual concentration of gas clouds, young clusters and OB associations (W3, W4 and W5). The small nebula S 201 is situated to the east of W5, which contains the young open cluster IC 1848. Probably associated with S 201 is one of the originally proposed Bok globules; the region also contains three infrared sources.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 211 - 212
Copyright
Copyright © Reidel 1987