Peculiar double-periodic pulsation in RR Lyrae stars of the
OGLE collection - II. Short-period stars with a dominant radial
fundamental mode

J 2017

Peculiar double-periodic pulsation in RR Lyrae stars of the OGLE collection - II. Short-period stars with a dominant radial fundamental mode

PRUDIL, Zdeněk; Radoslaw SMOLEC; Marek SKARKA a Henryka NETZEL

Základní údaje

Originální název

Peculiar double-periodic pulsation in RR Lyrae stars of the OGLE collection - II. Short-period stars with a dominant radial fundamental mode

Autoři

PRUDIL, Zdeněk; Radoslaw SMOLEC; Marek SKARKA a Henryka NETZEL

Vydání

Monthly Notices of the Royal Astronomical Society, Oxford, Oxford University Press, 2017, 0035-8711

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Velká Británie a Severní Irsko

Utajení

není předmětem státního či obchodního tajemství

Odkazy

Full Text

Impakt faktor

Impact factor: 5.194

Označené pro přenos do RIV

Ano

Kód RIV

RIV/00216224:14310/17:00108887

Organizační jednotka

Přírodovědecká fakulta

Klíčová slova anglicky

stars: horizontal branch; stars: oscillations; stars: variables: RR Lyrae; methods: data analysis

Štítky

rivok

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 24. 2. 2020 15:20, Mgr. Marie Novosadová Šípková, DiS.

Anotace

V originále

We report the discovery of a new group of double-periodic stars in the OGLE Galactic bulge photometry. In 38 stars identified as fundamental-mode RR Lyrae and four classified as firstovertone RR Lyrae, we detected an additional shorter periodicity. The periods of the dominant variability in the newly discovered group are 0.28 < P-D < 0.41 d. Period ratios (0.68-0.72) are smaller than the period ratios of the Galactic bulge RRd stars. The typical amplitude ratio (of the additional to the dominant periodicity) is 20 per cent for the stars identified as fundamental-mode RR Lyrae and 50 per cent for stars classified as first-overtone RR Lyrae. 10 stars from our sample exhibit equidistant peaks in the frequency spectrum, which suggests the Blazhko-type modulation of the main pulsation frequency and/ or additional periodicity. The Fourier coefficients R-21 and R-31 are some of the lowest among fundamental-mode RR Lyrae stars, but among the highest for the first-overtone pulsators. For the phase Fourier coefficients phi(21) and phi(31), our stars lie between RRab and RRc stars. The stars discussedwere compared with radial linear pulsation models. Their position in the Petersen diagram cannot be reproduced by assuming that two radial modes are excited and their physical parameters are like those characteristic of RR Lyrae stars. The non-radial-mode scenario also faces difficulties. We conclude that the dominant variability is most likely due to pulsation in the radial fundamental mode, which applies to stars classified as first-overtone mode pulsators. At this point, we cannot explain the nature of the additional periodicity. Even more, the classification of the stars as RR Lyrae should be treated as tentative.

Citovat

PRUDIL, Zdeněk; Radoslaw SMOLEC; Marek SKARKA a Henryka NETZEL. Peculiar double-periodic pulsation in RR Lyrae stars of the OGLE collection - II. Short-period stars with a dominant radial fundamental mode. Monthly Notices of the Royal Astronomical Society. Oxford: Oxford University Press, 2017, roč. 465, č. 4, s. 4074-4084. ISSN 0035-8711. Dostupné z: https://doi.org/10.1093/mnras/stw3010.

@article{1443980,
   author = {Prudil, Zdeněk and Smolec, Radoslaw and Skarka, Marek and Netzel, Henryka},
   article_location = {Oxford},
   article_number = {4},
   doi = {https://doi.org/10.1093/mnras/stw3010},
   keywords = {stars: horizontal branch; stars: oscillations; stars: variables: RR Lyrae; methods: data analysis},
   language = {eng},
   issn = {0035-8711},
   journal = {Monthly Notices of the Royal Astronomical Society},
   title = {Peculiar double-periodic pulsation in RR Lyrae stars of the OGLE collection - II. Short-period stars with a dominant radial fundamental mode},
   url = {https://academic.oup.com/mnras/article-abstract/465/4/4074/2736208?redirectedFrom=fulltext},
   volume = {465},
   year = {2017}
}

TY  - JOUR
ID  - 1443980
AU  - Prudil, Zdeněk - Smolec, Radoslaw - Skarka, Marek - Netzel, Henryka
PY  - 2017
TI  - Peculiar double-periodic pulsation in RR Lyrae stars of the OGLE collection - II. Short-period stars with a dominant radial fundamental mode
JF  - Monthly Notices of the Royal Astronomical Society
VL  - 465
IS  - 4
SP  - 4074-4084
EP  - 4074-4084
PB  - Oxford University Press
SN  - 00358711
KW  - stars: horizontal branch
KW  - stars: oscillations
KW  - stars: variables: RR Lyrae
KW  - methods: data analysis
UR  - https://academic.oup.com/mnras/article-abstract/465/4/4074/2736208?redirectedFrom=fulltext
L2  - https://academic.oup.com/mnras/article-abstract/465/4/4074/2736208?redirectedFrom=fulltext
N2  - We report the discovery of a new group of double-periodic stars in the OGLE Galactic bulge photometry. In 38 stars identified as fundamental-mode RR Lyrae and four classified as firstovertone RR Lyrae, we detected an additional shorter periodicity. The periods of the dominant variability in the newly discovered group are 0.28 < P-D < 0.41 d. Period ratios (0.68-0.72) are smaller than the period ratios of the Galactic bulge RRd stars. The typical amplitude ratio (of the additional to the dominant periodicity) is 20 per cent for the stars identified as fundamental-mode RR Lyrae and 50 per cent for stars classified as first-overtone RR Lyrae. 10 stars from our sample exhibit equidistant peaks in the frequency spectrum, which suggests the Blazhko-type modulation of the main pulsation frequency and/ or additional periodicity. The Fourier coefficients R-21 and R-31 are some of the lowest among fundamental-mode RR Lyrae stars, but among the highest for the first-overtone pulsators. For the phase Fourier coefficients phi(21) and phi(31), our stars lie between RRab and RRc stars. The stars discussedwere compared with radial linear pulsation models. Their position in the Petersen diagram cannot be reproduced by assuming that two radial modes are excited and their physical parameters are like those characteristic of RR Lyrae stars. The non-radial-mode scenario also faces difficulties. We conclude that the dominant variability is most likely due to pulsation in the radial fundamental mode, which applies to stars classified as first-overtone mode pulsators. At this point, we cannot explain the nature of the additional periodicity. Even more, the classification of the stars as RR Lyrae should be treated as tentative.
ER  -

PRUDIL, Zdeněk; Radoslaw SMOLEC; Marek SKARKA a Henryka NETZEL. Peculiar double-periodic pulsation in RR Lyrae stars of the OGLE collection - II. Short-period stars with a dominant radial fundamental mode. \textit{Monthly Notices of the Royal Astronomical Society}. Oxford: Oxford University Press, 2017, roč.~465, č.~4, s.~4074-4084. ISSN~0035-8711. Dostupné z: https://doi.org/10.1093/mnras/stw3010.

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