A study of the wind of P Cygni applying the self-absorption-curve method

Bibcode
2001ASPC..233..113F
Friedjung, M.; Muratorio, G.; Markova, N.; Israelian, G.
Referencia bibliográfica

P Cygni 2000: 400 Years of Progress, ASP Conference Proceeding Vol. 233, Edited by M. de Groot and C. Sterken, San Francisco: Astronomical Society of the Pacific. ISBN: 1-58381-070-6, 2001, p. 113.

Fecha de publicación:
6
2001
Número de autores
4
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
After a brief description of how spectral emission lines can be studied by the self-absorption-curve method, we show what happens when it is used to examine the FeIII and NII lines of P Cygni. An extremely surprising result is obtained; more highly-excited pure-emission lines without blueshifted absorption appear to be optically thicker than less-excited lines with blueshifted absorption. Such an effect is understandable if there are inhomogeneities in the wind.
Tipo
Sin árbitro

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