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Chemical Abundances in the Interstellar Medium of Galaxies from Spectrophotometry of Supernova Remnants

Published online by Cambridge University Press:  04 August 2017

S. D'Odorico  and
M. Dopita
S. D'Odorico
Affiliation:
European Southern Observatory, 8046 Garching bei München, West Germany
M. Dopita
Affiliation:
Mount Stromlo and Siding Spring Observatory, Australian National University, Camberra, Australia

Extract

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In the recent past supernova remnants (SNR) have been identified in external galaxies as far as 5 Mpc. These galaxies are: M 33(12), M 31(12), NGC 6822(1), IC 1613(1), NGC 2403(2), NGC 300 (2), NGC 4449(1), where the numbers of SNR confirmed by optical spectroscopy are given in parenthesis. Data for objects in the Magellanic Clouds are discussed extensively elsewhere in this volume.

Type
VI. Supernova Remnants in Other Galaxies
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 517 - 524
Copyright
Copyright © Reidel 1983 

References

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