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Natural quenching of stellar formation

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dc.contributor Salvador Solé, Eduard
dc.creator Alfaro Rudilla, Víctor
dc.date 2018-09-26T15:14:25Z
dc.date 2018-09-26T15:14:25Z
dc.date 2018-06
dc.date.accessioned 2024-12-16T10:26:43Z
dc.date.available 2024-12-16T10:26:43Z
dc.identifier http://hdl.handle.net/2445/124843
dc.identifier.uri http://fima-docencia.ub.edu:8080/xmlui/handle/123456789/21464
dc.description Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2018, Tutor: Eduard Salvador Solé
dc.description Observation shows that, over cosmic history, star formation increased until z = 2. After that it su ered a strong quenching. Various internal and external causes have been postulated to explain this phenomenon. In this paper, we investigate a third more fundamental possibility, which we call \natural quenching". This quenching would simply arise as the consequence of the growth of halos. According to numerical simulations, the more massive halos, the less concentrated they are so that the gas trapped within them cools at a lower rate. Consequently, over cosmic evolution, the accretion of gas onto galaxies slows down, which translates into a lower star formation rate. The aim of this study is to find the characteristic time at which this natural quenching becomes effective and check whether it coincides with a redshift of about 2.
dc.format 4 p.
dc.format application/pdf
dc.language eng
dc.rights cc-by-nc-nd (c) Alfaro, 2018
dc.rights http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.rights info:eu-repo/semantics/openAccess
dc.source Treballs Finals de Grau (TFG) - Física
dc.subject Formació d'estels
dc.subject Halos (Meteorologia)
dc.subject Treballs de fi de grau
dc.subject Star formation
dc.subject Halos (Meteorology)
dc.subject Bachelor's theses
dc.title Natural quenching of stellar formation
dc.type info:eu-repo/semantics/bachelorThesis


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