Tracing Physical Processes Affecting Spectral Formation in the Low-luminosity B[e] Stars of the FS CMa Group
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F19%3A10406184" target="_blank" >RIV/00216208:11320/19:10406184 - isvavai.cz</a>
Alternative codes found
RIV/00216224:14310/19:00113732
Result on the web
—
DOI - Digital Object Identifier
—
Alternative languages
Result language
angličtina
Original language name
Tracing Physical Processes Affecting Spectral Formation in the Low-luminosity B[e] Stars of the FS CMa Group
Original language description
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.
Czech name
—
Czech description
—
Classification
Type
D - Article in proceedings
CEP classification
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GA17-00871S" target="_blank" >GA17-00871S: Properties of the circumstellar matter around B[e] stars</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
RADIATIVE SIGNATURES FROM THE COSMOS
ISBN
978-1-58381-925-8
ISSN
1050-3390
e-ISSN
—
Number of pages
6
Pages from-to
155-160
Publisher name
ASTRONOMICAL SOC PACIFIC
Place of publication
SAN FRANCISCO
Event location
Sorbonne Univ
Event date
Oct 23, 2018
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000494866300024