Radio observations of P Cygni

Details Radio observations of P Cygni Radio observations of P Cygni

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aspc..233..241e&link_type=abstract

P Cygni 2000: 400 Years of Progress, ASP Conference Proceeding Vol. 233, Edited by M. de Groot and C. Sterken, San Francisco: As

Astronomy and Astrophysics

Astronomy

Scientific paper

In this paper the history of the radio study of P Cygni is summarized, concentrating on the observations rather than detailed physical modelling. P Cygni has been observed with radio arrays and single dishes on-and-off over the years. Its emission conforms largely to the model of a thermal free-free wind, with the addition of fainter extended nebulosity. Observations of increasing spatial resolution and sensitivity have revealed that the wind and circumstellar environment are variable and inhomogeneous.

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