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Massive star formation and chemical evolution in NGC 1313

Published online by Cambridge University Press:  07 August 2017

S.D. Ryder
S.D. Ryder*
Affiliation:
Mt Stromlo and Siding Spring Observatories The Australian National University Weston Creek P.O. ACT 2611 Australia

Extract

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The galaxy NGC 1313 is a late-type (almost Magellanic) barred spiral located midway between the Magellanic Clouds but at a distance of about 4.5 Mpc (de Vaucouleurs 1963). A comprehensive imaging and spectrophotometry program has been carried out in order to investigate the peculiar kinematics of NGC 1313 (Marcelin and Athanassoula 1982), as well as to study the relationships between the formation of massive stars and light element chemical abundances in spiral galaxies.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 481
Copyright
Copyright © Kluwer 

References

Kennicutt, R.C.: 1983, Ap. J. 272, 54.Google Scholar
Marcelin, M. and Athanassoula, E.: 1982, Astr. Ap. 105, 76.Google Scholar
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de Vaucouleurs, G.: 1963, Ap. J. 137, 720.Google Scholar