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Wolf-Rayet Stars Featured in Emission-Line Galaxies

Published online by Cambridge University Press:  14 August 2015

D. Kunth
D. Kunth*
Affiliation:
Institut d'Astrophysique, 98 bis Bld Arago, 75014 Paris, France

Extract

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Emission-line galaxies contain a large number of hot stars responsible for the emissive gas. They offer the opportunity of investigating the initial mass function of stars in regions of active star formation. So far, only integral properties of the ionizing complexes in giant H II regions or emission-line galaxies have been used (Lequeux et al., 1981) but no direct emission-line stellar feature has been thoroughly analyzed.

Type
SESSION 8 — X-RAY DATA — MISCELLANEOUS TOPICS — GENERAL DISCUSSION
Information
Symposium - International Astronomical Union , Volume 99: Wolf-Rayet Stars: Observations, Physics, Evolution , 1982 , pp. 569 - 570
Copyright
Copyright © Reidel 1982 

References

Conti, P.S., Massey, P.:1981, Astrophys. J. in press.Google Scholar
Kunth, D., Sargent, W.L.W.: 1981, Astron. Astrophys. 101, L5.Google Scholar
Lequeux, J., Maucherat-Joubert, M., Deharveng, J.M., Kunth, D.:1981, Astron. Astrophys. in press.Google Scholar