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undergraduate thesis
Mladi skupovi zvijezda
2022. urn:nbn:hr:166:596549
Boić, Stella
University of Split
Faculty of Science
Department of Physics

Cite this document

Boić, S. (2022). Mladi skupovi zvijezda (Undergraduate thesis). Split: University of Split, Faculty of Science. Retrieved from https://urn.nsk.hr/urn:nbn:hr:166:596549

Boić, Stella. "Mladi skupovi zvijezda." Undergraduate thesis, University of Split, Faculty of Science, 2022. https://urn.nsk.hr/urn:nbn:hr:166:596549

Boić, Stella. "Mladi skupovi zvijezda." Undergraduate thesis, University of Split, Faculty of Science, 2022. https://urn.nsk.hr/urn:nbn:hr:166:596549

Boić, S. (2022). 'Mladi skupovi zvijezda', Undergraduate thesis, University of Split, Faculty of Science, accessed 14 November 2024, https://urn.nsk.hr/urn:nbn:hr:166:596549

Boić S. Mladi skupovi zvijezda [Undergraduate thesis]. Split: University of Split, Faculty of Science; 2022 [cited 2024 November 14] Available at: https://urn.nsk.hr/urn:nbn:hr:166:596549

S. Boić, "Mladi skupovi zvijezda", Undergraduate thesis, University of Split, Faculty of Science, Split, 2022. Available at: https://urn.nsk.hr/urn:nbn:hr:166:596549

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Metadata
TitleMladi skupovi zvijezda
Title (english)Young stellar clusters
AuthorStella Boić
MentorMarko Kovač (mentor)
MentorTamara Rom (pomoć pri izradi, neposredni voditelj)
Committee memberMarko Kovač (predsjednik povjerenstva)
Committee memberKoraljka Mužić (član povjerenstva)
Committee memberTamara Rom (član povjerenstva)
GranterUniversity of Split
Faculty of Science
(Department of Physics)
Split
Defense date and country2022-09-23, Croatia
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract
Mladi skupovi zvijezda su otvorena zvjezdana jata koja su se formirala u posljednjih deset do nekoliko stotina milijuna godina. Nastaju na krakovima spiralnih galaksija u galaktičkoj ravnini te su nepravilnog oblika zbog slabe gravitacijske sile. Zvijezde istog skupa nastale su u isto vrijeme te dijele razna ista svojstva koja nam omogućavaju da utvrdimo je li neka zvijezda dio skupa. Jedan od najsvjetlijih i najbližih mladih skupova Zemlji je skup M45 ili Plejade. Koristeći paralaksu, apsolutnu i prividnu magnitudu te fitanjem ovih vrijednosti na izohrone određene starosti računamo broj članova, udaljenost i starost skupa Plejada. Dobivene vrijednosti jako malo odstupaju od literature te iz toga zaključujemo da je ovaj skup pogodan za korištenje kod računanja udaljenosti daljnjih nebeskih objekata.
Abstract (english)
Young star clusters are open star clusters that have formed in the last ten to several hundred million years. They are formed on the arms of spiral galaxies in the galactic plane and have an irregular shape due to the weak gravitational force. Stars in the same cluster are formed at the same time and share many of the same properties that allow us to determine whether a star is part of a cluster. One of the brightest and closest young clusters to Earth is the M45 or Pleiades cluster. Using parallax, absolute and apparent magnitude and by fitting these values to isochrones of a certain age, we calculate the number of members, distance and age of the Pleiades cluster. The obtained values deviate very little from the literature, and from this we conclude that this set is suitable for use when calculating the distance of further celestial objects.
Keywords
Keywords (english)
Languagecroatian
URN:NBNurn:nbn:hr:166:596549
Study programmeTitle: Physics
Study programme type: university
Study level: undergraduate
Academic / professional title: sveučilišni/a prvostupnik/prvostupnica (baccalaureus/baccalaurea) fizike (sveučilišni/a prvostupnik/prvostupnica (baccalaureus/baccalaurea) fizike)
Type of resourceText
File originBorn digital
Access conditionsOpen access
Terms of useLicence Attribution 4.0 International (CC BY 4.0) icon
Created on2023-02-07 14:57:04