Binary fraction of magnetic chemically peculiar stars

J 2020

Binary fraction of magnetic chemically peculiar stars

PAUNZEN, Ernst

Základní údaje

Originální název

Binary fraction of magnetic chemically peculiar stars

Autoři

PAUNZEN, Ernst (40 Rakousko, garant, domácí)

Vydání

Contributions of the Astronomical Observatory Skalnaté Pleso, Tatranská Lomnica, Astronomical Institute, Slovak Academy of Sciences, 2020, 1335-1842

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Slovensko

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL

Impakt faktor

Impact factor: 0.316

Kód RIV

RIV/00216224:14310/20:00115734

Organizační jednotka

Přírodovědecká fakulta

DOI

http://dx.doi.org/10.31577/caosp.2020.50.2.570

UT WoS

000523574300041

Klíčová slova anglicky

binaries: general; stars: chemically peculiar; stars: magnetic fields

Štítky

rivok

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 24. 11. 2020 13:21, Mgr. Marie Šípková, DiS.

Anotace

V originále

Magnetic chemically peculiar stars of the upper main sequence are slowly rotating early B to early F-type objects with elemental overabundances of several orders of magnitude compared to the Sun. The driving mechanism is diffusion in the calm stellar atmosphere intensified by the presence of a stable organized magnetic field. The binary fraction is vital to understanding the formation and evolution of these objects as well as possible operating angular momentum loss mechanisms. The available literature on the binary fraction is reviewed and a list of needed future working steps is presented.

Citovat

PAUNZEN, Ernst. Binary fraction of magnetic chemically peculiar stars. Contributions of the Astronomical Observatory Skalnaté Pleso. Tatranská Lomnica: Astronomical Institute, Slovak Academy of Sciences, 2020, roč. 50, č. 2, s. 570-573. ISSN 1335-1842. Dostupné z: https://dx.doi.org/10.31577/caosp.2020.50.2.570.

@article{1660102,
   author = {Paunzen, Ernst},
   article_location = {Tatranská Lomnica},
   article_number = {2},
   doi = {http://dx.doi.org/10.31577/caosp.2020.50.2.570},
   keywords = {binaries: general; stars: chemically peculiar; stars: magnetic fields},
   language = {eng},
   issn = {1335-1842},
   journal = {Contributions of the Astronomical Observatory Skalnaté Pleso},
   title = {Binary fraction of magnetic chemically peculiar stars},
   url = {http://www.astro.sk/caosp/Eedition/FullTexts/vol50no2/pp570-573.pdf},
   volume = {50},
   year = {2020}
}

TY  - JOUR
ID  - 1660102
AU  - Paunzen, Ernst
PY  - 2020
TI  - Binary fraction of magnetic chemically peculiar stars
JF  - Contributions of the Astronomical Observatory Skalnaté Pleso
VL  - 50
IS  - 2
SP  - 570-573
EP  - 570-573
PB  - Astronomical Institute, Slovak Academy of Sciences
SN  - 13351842
KW  - binaries: general
KW  - stars: chemically peculiar
KW  - stars: magnetic fields
UR  - http://www.astro.sk/caosp/Eedition/FullTexts/vol50no2/pp570-573.pdf
L2  - http://www.astro.sk/caosp/Eedition/FullTexts/vol50no2/pp570-573.pdf
N2  - Magnetic chemically peculiar stars of the upper main sequence are slowly rotating early B to early F-type objects with elemental overabundances of several orders of magnitude compared to the Sun. The driving mechanism is diffusion in the calm stellar atmosphere intensified by the presence of a stable organized magnetic field. The binary fraction is vital to understanding the formation and evolution of these objects as well as possible operating angular momentum loss mechanisms. The available literature on the binary fraction is reviewed and a list of needed future working steps is presented.
ER  -

PAUNZEN, Ernst. Binary fraction of magnetic chemically peculiar stars. \textit{Contributions of the Astronomical Observatory Skalnaté Pleso}. Tatranská Lomnica: Astronomical Institute, Slovak Academy of Sciences, 2020, roč.~50, č.~2, s.~570-573. ISSN~1335-1842. Dostupné z: https://dx.doi.org/10.31577/caosp.2020.50.2.570.

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