A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2020; you can also visit the original URL.
The file type is application/pdf.
The detection of a circumstellar shell around P Cygni by direct CCD imaging
1987
Symposium - International astronomical union
Preserved Fulltext
The star P Cygni (=HD 193237) is the proto-type of a class of stars with peculiar spectra, the so-called P-Cygni-stars (or Luminous Blue Variables). They are characterized by extreme mass-loss characteristics and wind densities surpassed only by the winds of Wolf-Rayet stars.
doi:10.1017/s0074180900156906
fatcat:lv57o6zlc5adtgqbylxh7eq33y