Large Magellanic Cloud loop nebulae and their stellar contents

Details Large Magellanic Cloud loop nebulae and their stellar contents Large Magellanic Cloud loop nebulae and their stellar contents

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..69..495g&link_type=abstract

Astrophysics and Space Science, vol. 69, no. 2, May 1980, p. 495-503.

Astronomy and Astrophysics

Astrophysics

4

Emission Spectra, Late Stars, Magellanic Clouds, Nebulae, Star Distribution, Stellar Spectra, Astronomical Photography, Diameters, Energy Distribution, Linear Equations, Star Clusters, Stellar Luminosity

Scientific paper

Linear correlations between the log of the diameter of ring-shaped nebulae and the log of the total number of embedded stars for two absolute magnitude levels of -2 and +2 magnitudes for the LMC have been found. This shows that less luminous stars are also contributing towards the illumination of the nebulae. A method for the determination of relative ages of these loop nebulae is described.

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