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Tracing Physical Processes Affecting Spectral Formation in the Low-luminosity B[e] Stars of the FS CMa Group

Publikace na Matematicko-fyzikální fakulta |
2019

Tento text není v aktuálním jazyce dostupný. Zobrazuje se verze "en".Abstrakt

In order to help model the circumstellar environment of FS CMa stars, we summarize the spectral features of these objects and point to physical phenomena that affect the structure of the circumstellar region.