Structure and Behavior of Ionized Stellar Winds

Details Structure and Behavior of Ionized Stellar Winds Structure and Behavior of Ionized Stellar Winds

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..227c&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

Radio Continuum: Stars, Stars: Individual (P Cyg, Cyg Ob2 No.12, Wr 147), Stars: Stellar Winds

Scientific paper

During the last decade the standard model assumptions (a steady, isotropic and homogeneous wind) have been questioned. We present a set of new VLA observations at 3.6 and 6 cm for P Cyg, Cyg OB2 No. 12 and WR 147. These objects have been reported to possess winds that may deviate from these basic assumptions. We discuss preliminary results for each source.

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