Theory and observations of two stars undergoing strong interaction
Název práce v češtině: | Teorie a pozorování silných interakcí dvojhvězd |
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Název v anglickém jazyce: | Theory and observations of two stars undergoing strong interaction |
Klíčová slova: | dvojhvězdy|vývoj hvězd|Kataklyzmické dvojhvězdy|červení veleobri|hydrodynamika|fotometrie|spektroskopie |
Klíčová slova anglicky: | binary stars|stellar evolution|cataclysmic variables|red supergiants|hydrodynamics|photometry|spectroscopy |
Akademický rok vypsání: | 2020/2021 |
Typ práce: | disertační práce |
Jazyk práce: | angličtina |
Ústav: | Ústav teoretické fyziky (32-UTF) |
Vedoucí / školitel: | doc. Mgr. Ondřej Pejcha, Ph.D. |
Řešitel: | skrytý - zadáno a potvrzeno stud. odd. |
Datum přihlášení: | 08.09.2020 |
Datum zadání: | 08.09.2020 |
Datum potvrzení stud. oddělením: | 01.10.2020 |
Datum a čas obhajoby: | 27.08.2024 11:00 |
Datum odevzdání elektronické podoby: | 21.06.2024 |
Datum odevzdání tištěné podoby: | 21.06.2024 |
Datum proběhlé obhajoby: | 27.08.2024 |
Oponenti: | Dr. Stephen Justham |
prof. Shazrene S. Mohamed | |
Zásady pro vypracování |
The goal of the thesis is to significantly develop understanding of the theory and observational implications of two stars undergoing strong interaction or a merger. Depending on the interests of the student, the work will focus on understanding unusual transients likely associated with binary star interactions, transients from stellar collisions, formation of dust and molecules in binary interactions, and understanding the observational implications of the theory (blue stragglers, R CrB stars, FK Com stars, eta Car, progenitor of SN1987A, etc.). In addition to analytic or semi-analytic work, the thesis can utilize existing codes or codes under development in the group: 1D stellar evolution, smoothed particle (radiation)hydrodynamics, moving mesh radiation hydrodynamics, or N-body calculations. In addition, the group is a member of All-Sky Automated Survey for Supernovae (ASAS-SN), and the thesis can include significant observational or data analysis component from ASAS-SN or other photometric or spectroscopic surveys (APOGEE, Gaia, TESS). |
Seznam odborné literatury |
Evolutionary Processes in Binary and Multiple Stars, by Peter Eggleton, pp. . ISBN 0521855578. Cambridge, UK: Cambridge University Press, 2006.
Statistics, Data Mining, and Machine Learning in Astronomy, by Z. Ivencić et al. Princeton, NJ: Princeton University Press, 2014 Morris, T., Podsiadlowski, P. 2007. The Triple-Ring Nebula Around SN 1987A: Fingerprint of a Binary Merger. Science 315, 1103. Naoz, S. 2016. The Eccentric Kozai-Lidov Effect and Its Applications. Annual Review of Astronomy and Astrophysics 54, 441. Pawlak, M., and 14 colleagues 2019. The ASAS-SN catalogue of variable stars - IV. Periodic variables in the APOGEE survey. Monthly Notices of the Royal Astronomical Society 487, 5932. Smith, N., and 9 colleagues 2018. Light echoes from the plateau in Eta Carinae's Great Eruption reveal a two-stage shock-powered event. Monthly Notices of the Royal Astronomical Society 480, 1466. "Cool and luminous transients from mass-losing binary stars" (http://adsabs.harvard.edu/abs/2016MNRAS.455.4351P) "Pre-explosion Spiral Mass Loss of a Binary Star Merger" (http://adsabs.harvard.edu/abs/2017ApJ...850...59P) "Shock-powered light curves of luminous red novae as signatures of pre-dynamical mass-loss in stellar mergers" (http://adsabs.harvard.edu/abs/2017MNRAS.471.3200M |
Předběžná náplň práce v anglickém jazyce |
There is now renewed interest in the evolution and death of binary stars connected with the detection of gravitational waves from double compact objects and the exploration of new time-domain phenomena. |