Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-25T02:59:36.804Z Has data issue: false hasContentIssue false
  • English
  • Français

The H-R Diagram of NGC 1962-65-66-70

Published online by Cambridge University Press:  04 August 2017

E. Schulz-Lüpertz  and
M. Grewing
E. Schulz-Lüpertz
Affiliation:
Astronomisches Institut der Universität Tübingen Space Sciences Laboratory, University of California, Berkeley
M. Grewing
Affiliation:
Astronomisches Institut der Universität Tübingen

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 complex NGC 1962–65–66–70 is one of the many giant filamentary shell nebulae in the LMC. The nebulosity, also known as N144 was studied originally in H-alpha by Henize (1956). It has an angular size of 698″ x 620″ and surrounds an association of very young blue stars. The cluster has been studied first photographically in V and B by Westerlund (1961).

Type
Magellanic Cloud Clusters
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 35 - 36
Copyright
Copyright © Reidel 1984 

References

Grewing, M., Schulz-Lüpertz, E. 1980, Proc. 2nd Europ. IUE Conf., ESA SP-157, 357 Google Scholar
Henize, K.G. 1956, Astrophys. J. Suppl. 2, 315 Google Scholar
Maeder, A. 1981, Astron. Astrophys. 99, 97, and Astron. Astrophys. 102, 401 Google Scholar
Schmidt-Kaler, Th. 1982, Landolt-Börnstein Vol. 2b, eds. Schaifers, K., Voigt, H.H. Google Scholar
Schulz-Lüpertz, E., Grewing, M. 1982, Mitt. Astron. Ges. 55, 123 Google Scholar
Schulz-Lüpertz, E., Grewing, M. 1983, Astron. Astrophys. (submitted) Google Scholar
Westerlund, B. 1961, Uppsala Astronom. Obs. Ann. 5, no. 1 Google Scholar