2019
An Overview of the Properties of a Sample of Newly-Identified Magnetic Chemically Peculiar Stars in the Kepler Field
MIKULÁŠEK, Zdeněk; Ernst PAUNZEN; Stephan HUMMERICH; Jan JANÍK; Klaus BERNHARD et al.Základní údaje
Originální název
An Overview of the Properties of a Sample of Newly-Identified Magnetic Chemically Peculiar Stars in the Kepler Field
Autoři
MIKULÁŠEK, Zdeněk; Ernst PAUNZEN; Stephan HUMMERICH; Jan JANÍK ORCID; Klaus BERNHARD; Jiří KRTIČKA a Iliya YAKUNIN
Vydání
518. vyd. SAN FRANCISCO, Astronomical Society of the Pacific Conference Series, od s. 117-124, 8 s. 2019
Nakladatel
ASTRONOMICAL SOC PACIFIC
Další údaje
Jazyk
angličtina
Typ výsledku
Stať ve sborníku
Obor
10308 Astronomy
Stát vydavatele
Spojené státy
Utajení
není předmětem státního či obchodního tajemství
Forma vydání
tištěná verze "print"
Odkazy
Označené pro přenos do RIV
Ano
Kód RIV
RIV/00216224:14310/19:00107581
Organizační jednotka
Přírodovědecká fakulta
ISBN
978-1-58381-924-1
ISSN
UT WoS
Klíčová slova česky
Kepler photometry; chemically peculiar stars;
Klíčová slova anglicky
Kepler photometry; chemically peculiar stars;
Štítky
Příznaky
Mezinárodní význam, Recenzováno
Změněno: 24. 3. 2020 11:52, Mgr. Marie Novosadová Šípková, DiS.
V originále
We present a comprehensive overview of the properties of a sample of 41 magnetic chemically peculiar stars that have been recently identified in the Kepler field by our team. The stars populate the whole age range from the zero-age to terminal-age main sequence in a mass interval from 1.5 to 4 M-circle dot. Several of the studied objects exhibit a hitherto unobserved wealth of detail in their light curves indicative of persisting complex surface structures. Monoperiodic variability and light curve stability were identified as cardinal criteria for selecting mCP star candidates among early-type objects in photometric surveys. Subsequent studies will be concerned with an exhaustive follow-up analysis of the new mCP stars, which we expect to lead to new insights on the physics of the CP star phenomenon.
Česky
We present a comprehensive overview of the properties of a sample of 41 magnetic chemically peculiar stars that have been recently identified in the Kepler field by our team. The stars populate the whole age range from the zero-age to terminal-age main sequence in a mass interval from 1.5 to 4 M-circle dot. Several of the studied objects exhibit a hitherto unobserved wealth of detail in their light curves indicative of persisting complex surface structures. Monoperiodic variability and light curve stability were identified as cardinal criteria for selecting mCP star candidates among early-type objects in photometric surveys. Subsequent studies will be concerned with an exhaustive follow-up analysis of the new mCP stars, which we expect to lead to new insights on the physics of the CP star phenomenon.
Návaznosti
| GA16-01116S, projekt VaV |
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