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

0520217 - ASÚ 2020 RIV US eng C - Konferenční příspěvek (zahraniční konf.)
Korčáková, D. - Shore, S. N. - Miroshnichenko, A. S. - Zharikov, S.V. - Jeřábková, T. - Dvořáková, N. - Votruba, V. - Manset, N. - Šlechta, Miroslav
Tracing Physical Processes Affecting Spectral Formation in the Low-luminosity B[e] Stars of the FS CMa Group.
Radiative Signatures from the Cosmos: A Conference in Honor of Ivan Hubený. San Francisco: Astronomical Society of the Pacific, 2019 - (Werner, K.), s. 155-150. ASP Conference Series, 519. ISBN 9781583819265. ISSN 1050-3390.
[Conference on Radiative Signatures from the Cosmos. Paris (FR), 23.10.2018-26.10.2018]
Grant ostatní: GA ČR(CZ) GA17-00871S
Institucionální podpora: RVO:67985815
Klíčová slova: FS CMa stars * model the circumstellar environment * spectral features
Obor OECD: Astronomy (including astrophysics,space science)

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.
Trvalý link: http://hdl.handle.net/11104/0304905