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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

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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