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Soriano, Mélanie. "Astérosismologie d'étoiles de séquence principale ou évoluées en relation avec l'expérience spatiale COROT et les instruments au sol HARPS et SOPHIE". Toulouse 3, 2009. http://thesesups.ups-tlse.fr/827/.
Pełny tekst źródłaThe work presented in this thesis focuses on asteroseismology of solar-type stars, and more specifically on central stars of planetary systems. The analysis of waves propagating in these stars can help constraining their internal structure. The two first chapters describe the theory and the stellar oscillations and the numerical tools used for this work. The third part deals with HD 52265, target of the CoRoT mission with a planet. We computed preliminary models for this star, taking into account the spectroscopic constraints, and we made some asteroseismic predictions. During this study, we found a seismic signature characteristic of the stellar core. This phenomenon is induced by a strong helium gradient in the core. We studied this effect in the general case of solar-type stars and we showed that it always happens, at the end of the main sequence or at the beginning of the subgiant branch. This characteristic signature can be used to constrain the stellar core. The fifth chapter is devoted to the star 51 Peg. We observed this star with the SOPHIE spectrograph at the Observatoire de Haute Provence in 2007 and we detected its oscillations. The analysis of the data led to the identification of 21 pulsation modes. Finally, we present a new seismic analysis of the exoplanet-host star µ Arae, observed and analysed by Bazot et al. In 2004. Asteroseismology coupled with spectroscopy allowed us to determine the helium abundance of the star, and its parameters: mass, age, radius, size of the convective core and its possible extension due to overshooting. These results show that asteroseismology is a powerful tool to bring constraints on the internal structure of stars
Soriano, Melanie. "Astérosismologie d'étoiles de séquence principale ou évoluées, en relation avec l'expérience spatiale CoRoT, et les instruments au sol HARPS et SOPHIE". Phd thesis, Université Paul Sabatier - Toulouse III, 2009. http://tel.archives-ouvertes.fr/tel-00438082.
Pełny tekst źródłaPhilipot, Florian. "Vers une recherche exhaustive des planètes géantes autour des étoiles proches de type solaire". Electronic Thesis or Diss., Université Paris sciences et lettres, 2023. http://www.theses.fr/2023UPSLO008.
Pełny tekst źródłaThe detection of the first exoplanets in the 1990s opened a new era in the study of planets. Today, thanks to increasingly powerful instruments, several hundred exoplanets (hot Jupiters, Super-Earths, multiple systems...) are discovered every year. Thanks to this wide variety of exoplanets, it is possible to study the distribution (distance, mass, eccentricity...) of these objects in order to better constrain the formation and evolution models of planetary system. Nevertheless, each detection method has its own limitations and detection biases. One aim of this thesis was to identify the limitations of the various detection methods, in particular those related to radial velocities (RV), and to improve the characterization of companions detected by RV.As a first step, I tested the robustness of studies aimed at determining the radial distribution of giant planets. Analysis of RV data from stars hosting long-period planets, the impact of stellar activity and the hypothesis made in completeness calculations, allowed us to demonstrate that statistical RV studies were not robust beyond 7-8 AU. Subsequently, I combined RV data with available absolute and relative astrometry measurements to improve the characterization of long-period sub-stellar companions. This study allowed us to precisely constrain the orbital parameters and, above all, the mass of seven companions detected in RV. It also highlighted the importance of coupling RV data with other measurements to accurately determine the nature of a companion. Finally, I used measurements of stars' proper motion anomalies (PMa), derived from Hipparcos and Gaia absolute astrometry, to search for new sub-stellar companions in the HARPS/VLT spectrograph archive. This analysis enabled me to improve the characterization of 14 sub-stellar companions, and to discover three new brown dwarfs and seven new exoplanets. I also demonstrated the effectiveness of using PMa measurements to optimize the search for sub-stellar companions
Santerne, Alexandre. "La caractérisation des exoplanètes en transit par vélocimétrie radiale". Thesis, Aix-Marseille, 2012. http://www.theses.fr/2012AIXM4800/document.
Pełny tekst źródłaThe search and characterization of transiting extrasolar planets (i.e. that pass in front of their host star, as seen from the Earth) is an important domain of planetology since these planets constrain the formation, evolution and migration process of planetary systems. The CoRoT (CNES) and Kepler (NASA) space missions permit, these last years, to discover several thousand of transiting-planet candidates. However, these planet candidates need to be confirmed in order to exclude all false positive scenario that can mimic a planetary transit. For that, one of the method consist on performing radial velocity follow-up observations to measure the transiting object's mass and orbital parameters and thus, to determine the nature of planet candidates.During my PhD thesis, I tried to resolve the nature of transiting planet candidates from the CoRoT and Kepler space missions. For that, I performed follow-up observations with the SOPHIE (OHP) and HARPS (ESO) spectrographs that were used to discover several new transiting extrasolar planets. I also measured the Kepler false-positive rate, equal to 35% for giant close-in exoplanet candidates, contradicting previous estimations, much more optimistic.I also participate to the development of a new software, called "PASTIS", which objective is to validate statistically low-mass transiting exoplanets out of reach for current spectrographs. This new tool will, in a near future, validate tens of low-mass planets from the CoRoT and Kepler space missions
Loeillet, Benoit. "Planètes extrasolaires à courte période orbitale: De la détection à la caractérisation des Jupiter-chauds". Phd thesis, Université de Provence - Aix-Marseille I, 2008. http://tel.archives-ouvertes.fr/tel-00353240.
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