| dc.contributor.advisor | Zasche, Petr | |
| dc.creator | Smorada, Filip | |
| dc.date.accessioned | 2024-11-28T14:24:41Z | |
| dc.date.available | 2024-11-28T14:24:41Z | |
| dc.date.issued | 2024 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.11956/193880 | |
| dc.description.abstract | Pulzujúce hviezdy majú premennú veľkosť, teplotu, farbu, atď. Tieto faktory zaprí- čiňujú zmenu množstva vyžarovaného svetla. Zmena je zvyčajne periodická a často sa skladá z viacerých frekvencií s rôznymi amplitúdami. Cieľom tejto práce je určenie frek- vencií pulzácií hviezd a následne porovnanie výsledkov získaných z rôznych meraní. 1 | cs_CZ |
| dc.description.abstract | Pulsating stars undergo changes, i.e. perpetual expansion and contraction, tempera- ture changes, color changes. These changes result in variations of emitted light. Variation is usually periodical and often consists of several disctinct processes with their respective frequencies and amplitudes. This thesis focuses on identifying pulsation frequencies of studied stars and comparing results acquried from data from different sources. 1 | en_US |
| dc.language | Slovenčina | cs_CZ |
| dc.language.iso | sk_SK | |
| dc.publisher | Univerzita Karlova, Matematicko-fyzikální fakulta | cs_CZ |
| dc.subject | pulsating variale stars|delta Scuti stars|TESS satellite | en_US |
| dc.subject | pulzující proměnné hvězdy|hvězdy typu delta Scuti|TESS satelit | cs_CZ |
| dc.title | Pulzujúce hviezdy v databáze TESS | sk_SK |
| dc.type | bakalářská práce | cs_CZ |
| dcterms.created | 2024 | |
| dcterms.dateAccepted | 2024-09-11 | |
| dc.description.department | Astronomical Institute of Charles University | en_US |
| dc.description.department | Astronomický ústav UK | cs_CZ |
| dc.description.faculty | Matematicko-fyzikální fakulta | cs_CZ |
| dc.description.faculty | Faculty of Mathematics and Physics | en_US |
| dc.identifier.repId | 262004 | |
| dc.title.translated | Pulsating stars from TESS database | en_US |
| dc.title.translated | Pulzující hvězdy z databáze TESS | cs_CZ |
| dc.contributor.referee | Harmanec, Petr | |
| thesis.degree.name | Bc. | |
| thesis.degree.level | bakalářské | cs_CZ |
| thesis.degree.discipline | Physics | en_US |
| thesis.degree.discipline | Fyzika | cs_CZ |
| thesis.degree.program | Physics | en_US |
| thesis.degree.program | Fyzika | cs_CZ |
| uk.thesis.type | bakalářská práce | cs_CZ |
| uk.taxonomy.organization-cs | Matematicko-fyzikální fakulta::Astronomický ústav UK | cs_CZ |
| uk.taxonomy.organization-en | Faculty of Mathematics and Physics::Astronomical Institute of Charles University | en_US |
| uk.faculty-name.cs | Matematicko-fyzikální fakulta | cs_CZ |
| uk.faculty-name.en | Faculty of Mathematics and Physics | en_US |
| uk.faculty-abbr.cs | MFF | cs_CZ |
| uk.degree-discipline.cs | Fyzika | cs_CZ |
| uk.degree-discipline.en | Physics | en_US |
| uk.degree-program.cs | Fyzika | cs_CZ |
| uk.degree-program.en | Physics | en_US |
| thesis.grade.cs | Velmi dobře | cs_CZ |
| thesis.grade.en | Very good | en_US |
| uk.abstract.cs | Pulzujúce hviezdy majú premennú veľkosť, teplotu, farbu, atď. Tieto faktory zaprí- čiňujú zmenu množstva vyžarovaného svetla. Zmena je zvyčajne periodická a často sa skladá z viacerých frekvencií s rôznymi amplitúdami. Cieľom tejto práce je určenie frek- vencií pulzácií hviezd a následne porovnanie výsledkov získaných z rôznych meraní. 1 | cs_CZ |
| uk.abstract.en | Pulsating stars undergo changes, i.e. perpetual expansion and contraction, tempera- ture changes, color changes. These changes result in variations of emitted light. Variation is usually periodical and often consists of several disctinct processes with their respective frequencies and amplitudes. This thesis focuses on identifying pulsation frequencies of studied stars and comparing results acquried from data from different sources. 1 | en_US |
| uk.file-availability | V | |
| uk.grantor | Univerzita Karlova, Matematicko-fyzikální fakulta, Astronomický ústav UK | cs_CZ |
| thesis.grade.code | 2 | |
| uk.publication-place | Praha | cs_CZ |
| uk.thesis.defenceStatus | O | |
