Photometric investigation of contact binaries near the short
period limit-1SWASPJ161335.80-284722.2

J 2019

Photometric investigation of contact binaries near the short period limit-1SWASPJ161335.80-284722.2

ZEJDA, Miloslav, S.B. QIAN, L.Y. ZHU a X.H. FANG

Základní údaje

Originální název

Photometric investigation of contact binaries near the short period limit-1SWASPJ161335.80-284722.2

Autoři

ZEJDA, Miloslav (203 Česká republika, garant, domácí), S.B. QIAN, L.Y. ZHU a X.H. FANG

Vydání

Contributions of the Astronomical Observatory Skalnaté Pleso, TATRANSKA LOMINICA, SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST, 2019, 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: 0.636

Kód RIV

RIV/00216224:14310/19:00108247

Organizační jednotka

Přírodovědecká fakulta

UT WoS

000469927500064

Klíčová slova anglicky

contact binary; photometry

Štítky

rivok

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 21. 4. 2020 17:25, Mgr. Marie Šípková, DiS.

Anotace

V originále

A new period distribution of W UMa type (EW) contact binaries indicates that the short-period limit for EWs is around 0.2 days. Close binary stars with orbital periods near to this limit are an important source to understand the formation and evolution of contact binaries. Recently, some close binary stars with orbital periods in the range of 0.2 to 0.23 days were monitored and their light curves were analyzed using the W-D method. We present here one example of such studies - an analysis of 1SWASPJ161335.80-284722.2, its photometric solutions and period changes.

Návaznosti

GA16-01116S, projekt VaV

Název: Atmosféry a okolohvězdné prostředí magnetických horkých hvězd

Investor: Grantová agentura ČR, Atmosféry a okolohvězdné prostředí magnetických horkých hvězd

Citovat

ZEJDA, Miloslav, S.B. QIAN, L.Y. ZHU a X.H. FANG. Photometric investigation of contact binaries near the short period limit-1SWASPJ161335.80-284722.2. Contributions of the Astronomical Observatory Skalnaté Pleso. TATRANSKA LOMINICA: SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST, 2019, roč. 49, č. 2, s. 453-455. ISSN 1335-1842.

@article{1642482,
   author = {Zejda, Miloslav and Qian, S.B. and Zhu, L.Y. and Fang, X.H.},
   article_location = {TATRANSKA LOMINICA},
   article_number = {2},
   keywords = {contact binary; photometry},
   language = {eng},
   issn = {1335-1842},
   journal = {Contributions of the Astronomical Observatory Skalnaté Pleso},
   title = {Photometric investigation of contact binaries near the short period limit-1SWASPJ161335.80-284722.2},
   url = {https://ui.adsabs.harvard.edu/abs/2019CoSka..49..453Z/abstract},
   volume = {49},
   year = {2019}
}

TY  - JOUR
ID  - 1642482
AU  - Zejda, Miloslav - Qian, S.B. - Zhu, L.Y. - Fang, X.H.
PY  - 2019
TI  - Photometric investigation of contact binaries near the short period limit-1SWASPJ161335.80-284722.2
JF  - Contributions of the Astronomical Observatory Skalnaté Pleso
VL  - 49
IS  - 2
SP  - 453-455
EP  - 453-455
PB  - SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST
SN  - 13351842
KW  - contact binary
KW  - photometry
UR  - https://ui.adsabs.harvard.edu/abs/2019CoSka..49..453Z/abstract
L2  - https://ui.adsabs.harvard.edu/abs/2019CoSka..49..453Z/abstract
N2  - A new period distribution of W UMa type (EW) contact binaries indicates that the short-period limit for EWs is around 0.2 days. Close binary stars with orbital periods near to this limit are an important source to understand the formation and evolution of contact binaries. Recently, some close binary stars with orbital periods in the range of 0.2 to 0.23 days were monitored and their light curves were analyzed using the W-D method. We present here one example of such studies - an analysis of 1SWASPJ161335.80-284722.2, its photometric solutions and period changes.
ER  -

ZEJDA, Miloslav, S.B. QIAN, L.Y. ZHU a X.H. FANG. Photometric investigation of contact binaries near the short period limit-1SWASPJ161335.80-284722.2. \textit{Contributions of the Astronomical Observatory Skalnaté Pleso}. TATRANSKA LOMINICA: SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST, 2019, roč.~49, č.~2, s.~453-455. ISSN~1335-1842.

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