Wolf-Rayet stars in extragalactic H II regions. II - NGC604 - A giant H II region dominated by many Wolf-Rayet stars

Details Wolf-Rayet stars in extragalactic H II regions. II - NGC604 - A giant H II region dominated by many Wolf-Rayet stars Wolf-Rayet stars in extragalactic H II regions. II - NGC604 - A giant H II region dominated by many Wolf-Rayet stars

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...108..339r&link_type=abstract

Astronomy and Astrophysics, vol. 108, no. 2, Apr. 1982, p. 339-343. Deutsche Forschungsgemeinschaft

Astronomy and Astrophysics

Astrophysics

41

H Ii Regions, Intergalactic Media, Stellar Winds, Wolf-Rayet Stars, Astronomical Spectroscopy, Bubbles, H Alpha Line, Interstellar Space, Ionized Gases, Kinematics, Kinetic Energy, Stellar Envelopes, Stellar Mass Ejection, Supersonic Speed

Scientific paper

The unusually large numbers of WR stars, the numerous shells of ionized
material and the supersonic motions observed in NGC 604 are discussed
within the theory of interstellar wind-driven bubbles. It is shown, that
the kinetic energies involved can be easily supplied by the strong mass
loss phenomena of the WR stars.

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