Article contents
Planetary nebulae and Wolf-Rayet stars in the Magellanic Clouds
Published online by Cambridge University Press: 14 August 2015
Extract
Objects in the Small Magellanic Cloud classified by Lindsay (1961) as planetary nebulae or probable planetary nebulae have been studied in detail on large-scale photographs (Henize and Westerlund 1963). Of Lindsay's 50 objects, 11 are clearly resolved, 2 are probably resolved, 12 show stellar images, 13 are below the limit of the plates, 11 (fairly faint) are outside the photographed regions, and 1 is of uncertain identification. The masses of the resolved nebulae lie between 2 and 33 solar masses. They are therefore classified as small diffuse nebulae; it appears unlikely that the mass of a planetary nebula can exceed a few tenths of a solar mass.
- Type
- Section II: The Magellanic Clouds
- Information
- Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 316 - 321
- Copyright
- Copyright © Australian Academy of Science 1964
References
- 7
- Cited by