No CrossRef data available.
Article contents
The H-R Diagram of NGC 1962-65-66-70
Published online by Cambridge University Press: 04 August 2017
Extract
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
- Copyright
- Copyright © Reidel 1984