Blazhko effect at the time of Kepler

D 2015

Blazhko effect at the time of Kepler

SKARKA, Marek

Základní údaje

Originální název

Blazhko effect at the time of Kepler

Autoři

SKARKA, Marek (203 Česká republika, garant, domácí)

Vydání

Czech Republic, Proceedings of the 46th Conference on Variable Stars Research, od s. 10-13, 4 s. 2015

Nakladatel

Sekce pozorovatelů proměnných hvězd České astronomické společnosti

Další údaje

Jazyk

angličtina

Typ výsledku

Stať ve sborníku

Obor

10308 Astronomy

Stát vydavatele

Česká republika

Utajení

není předmětem státního či obchodního tajemství

Forma vydání

elektronická verze "online"

Odkazy

URL

Kód RIV

RIV/00216224:14310/15:00082578

Organizační jednotka

Přírodovědecká fakulta

ISSN

Klíčová slova anglicky

Blazhko effect; RR Lyrae; Kepler satellite

Změněno: 31. 3. 2015 10:23, Mgr. Marek Skarka, Ph.D.

Anotace

V originále

I focus on the comparison of the knowledge of the enigmatic Blazhko phenomenon before and after space missions CoRoT and Kepler. These two telescopes opened the secret doors of the true diversity of the modulation of RR Lyrae stars. Among many interesting discoveries it was found that higher order multiplets are common characteristics of the frequency spectra of light curves of modulated stars, not unique behaviour of a few objects. This finding resulted in a new mathematical description of modulation which applies methods known from information transfer. Signs of higher radial modes and non-radial modes were detected only due to unprecedented precision of space observations. One of the most important discoveries of the Kepler satellite was the uncovering of the alternation of the height of maxima of light changes in modulated stars, the so called period doubling. Based on this new discovery models for explanation of the Blazhko effect were proposed. In addition, Kepler observations clearly showed that Blazhko effect can be irregular in many ways. Therefore, space missions have a major impact on understanding of the Blazhko effect.

Návaznosti

MUNI/A/0773/2013, interní kód MU

Název: Pokročilé problémy teoretické fyziky a astrofyziky

Investor: Masarykova univerzita, Pokročilé problémy teoretické fyziky a astrofyziky, DO R. 2020_Kategorie A - Specifický výzkum - Studentské výzkumné projekty

Citovat

SKARKA, Marek. Blazhko effect at the time of Kepler. Online. In Kocián, R. Proceedings of the 46th Conference on Variable Stars Research. Czech Republic: Sekce pozorovatelů proměnných hvězd České astronomické společnosti, 2015, s. 10-13. ISSN 1801-5964.

@inproceedings{1231595,
   author = {Skarka, Marek},
   address = {Czech Republic},
   booktitle = {Proceedings of the 46th Conference on Variable Stars Research},
   editor = {Kocián, R.},
   keywords = {Blazhko effect; RR Lyrae; Kepler satellite},
   howpublished = {elektronická verze "online"},
   language = {eng},
   location = {Czech Republic},
   pages = {10-13},
   publisher = {Sekce pozorovatelů proměnných hvězd České astronomické společnosti},
   title = {Blazhko effect at the time of Kepler},
   url = {http://var.astro.cz/oejv/issues/oejv0169.pdf},
   year = {2015}
}

TY  - JOUR
ID  - 1231595
AU  - Skarka, Marek
PY  - 2015
TI  - Blazhko effect at the time of Kepler
PB  - Sekce pozorovatelů proměnných hvězd České astronomické společnosti
CY  - Czech Republic
KW  - Blazhko effect
KW  - RR Lyrae
KW  - Kepler satellite
UR  - http://var.astro.cz/oejv/issues/oejv0169.pdf
N2  - I focus on the comparison of the knowledge of the enigmatic Blazhko phenomenon before and after space missions CoRoT and Kepler. These two telescopes opened the secret doors of the true diversity of the modulation of RR Lyrae stars. Among many interesting discoveries it was found that higher order multiplets are common characteristics of the frequency spectra of light curves of modulated stars, not unique behaviour of a few objects. This finding resulted in a new mathematical description of modulation which applies methods known from information transfer. Signs of higher radial modes and non-radial modes were detected only due to unprecedented precision of space observations. One of the most important discoveries of the Kepler satellite was the uncovering of the alternation of the height of maxima of light changes in modulated stars, the so called period doubling. Based on this new discovery models for explanation of the Blazhko effect were proposed. In addition, Kepler observations clearly showed that Blazhko effect can be irregular in many ways. Therefore, space missions have a major impact on understanding of the Blazhko effect.
ER  -

SKARKA, Marek. Blazhko effect at the time of Kepler. Online. In Kocián, R. \textit{Proceedings of the 46th Conference on Variable Stars Research}. Czech Republic: Sekce pozorovatelů proměnných hvězd České astronomické společnosti, 2015, s.~10-13. ISSN~1801-5964.

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