Dissertations / Theses on the topic 'Stars with planets'
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Barker, Adrian John. "Tidal interactions between planets and stars." Thesis, University of Cambridge, 2011. https://www.repository.cam.ac.uk/handle/1810/240581.
Full textOrtiz, Mauricio, Sabine Reffert, Trifon Trifonov, Andreas Quirrenbach, David S. Mitchell, Grzegorz Nowak, Esther Buenzli, et al. "Precise radial velocities of giant stars." EDP SCIENCES S A, 2016. http://hdl.handle.net/10150/622444.
Full textDaley-Yates, Simon. "Radio emission from hot stars and planets." Thesis, University of Birmingham, 2018. http://etheses.bham.ac.uk//id/eprint/8585/.
Full textJermyn, Adam Sean. "Turbulence and transport in stars and planets." Thesis, University of Cambridge, 2018. https://www.repository.cam.ac.uk/handle/1810/278021.
Full textWeldrake, David Thomas Fredrick, and weldrake@mpia-hd mpg de. "Giant Planets and Variable Stars in Globular Clusters." The Australian National University. Research School of Astronomy and Astrophysics, 2005. http://thesis.anu.edu.au./public/adt-ANU20050616.191315.
Full textWeldrake, David Thomas Frederick. "Giant planets and variable stars in globular clusters /." View thesis entry in Australian Digital Theses Program, 2005. http://thesis.anu.edu.au/public/adt-ANU20050616.191315/index.html.
Full textSainsbury-Martinez, Felix. "Flows, instabilities, and magnetism in stars and planets." Thesis, University of Exeter, 2017. http://hdl.handle.net/10871/32072.
Full textGrether, Daniel Andrew Physics Faculty of Science UNSW. "Statistical analyses of extrasolar planets and other close companions to nearby stars." Awarded by:University of New South Wales. School of Physics, 2006. http://handle.unsw.edu.au/1959.4/29182.
Full textPetigura, Erik Ardeshir. "Prevalence of Earth-size Planets Orbiting Sun-like Stars." Thesis, University of California, Berkeley, 2015. http://pqdtopen.proquest.com/#viewpdf?dispub=3720767.
Full textIn this thesis, I explore two topics in exoplanet science. The first is the prevalence of Earth-size planets in the Milky Way Galaxy. To determine the occurrence of planets having different sizes, orbital periods, and other properties, I conducted a survey of extrasolar planets using data collected by NASA’s Kepler Space Telescope. This project involved writing new algorithms to analyze Kepler data, finding planets, and conducting follow-up work using ground-based telescopes. I found that most stars have at least one planet at or within Earth’s orbit and that 26% of Sun-like stars have an Earth-size planet with an orbital period of 100 days or less.
The second topic is the connection between the properties of planets and their host stars. The precise characterization of exoplanet hosts helps to bring planet properties like mass, size, and equilibrium temperature into sharper focus and probes the physical processes that form planets. I studied the abundance of carbon and oxygen in over 1000 nearby stars using optical spectra taken by the California Planet Search. I found a large range in the relative abundance of carbon and oxygen in this sample, including a handful of carbon-rich stars. I also developed a new technique called SpecMatch for extracting fundamental stellar parameters from optical spectra. SpecMatch is particularly applicable to the relatively faint planet-hosting stars discovered by Kepler.
Gallardo, José. "Physics of low mass stars, brown dwarfs and extrasolar planets." Lyon, École normale supérieure (sciences), 2007. http://www.theses.fr/2007ENSL0412.
Full textHaywood, Raphaëlle D. "Hide and seek : radial-velocity searches for planets around active stars." Thesis, University of St Andrews, 2015. http://hdl.handle.net/10023/7798.
Full textJackson, Brian, Phil Arras, Kaloyan Penev, Sarah Peacock, and Pablo Marchant. "A New Model of Roche Lobe Overflow for Short-period Gaseous Planets and Binary Stars." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624385.
Full textDominis, Dijana. "The role of binary stars in searches for extrasolar planets by microlensing and astrometry." Phd thesis, Universität Potsdam, 2006. http://opus.kobv.de/ubp/volltexte/2006/1081/.
Full textKovács, Gábor. "Infrared variability studies of low-mass stars in the field and in the Carina Nebula star forming region." Thesis, University of Cambridge, 2015. https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.709097.
Full textOrtiz, Álvarez Mauricio [Verfasser], and Andreas [Akademischer Betreuer] Quirrenbach. "Planets around giant stars: Two close-in transiting planets and one S-type planet in an eccentric binary system / Mauricio Ortiz Álvarez ; Betreuer: Andreas Quirrenbach." Heidelberg : Universitätsbibliothek Heidelberg, 2017. http://d-nb.info/118073890X/34.
Full textBirkby, Jayne Louise. "Observational constraints on low-mass stellar evolution and planet formation." Thesis, University of Cambridge, 2012. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.610381.
Full textMelis, Carl Anthony. "The life, death, and composition of exoterrestrial planets around intermediate mass stars." Diss., Restricted to subscribing institutions, 2009. http://proquest.umi.com/pqdweb?did=1973727501&sid=1&Fmt=2&clientId=1564&RQT=309&VName=PQD.
Full textPope, Benjamin James Spinks. "Observing bright stars and their planets from the Earth and from space." Thesis, University of Oxford, 2017. https://ora.ox.ac.uk/objects/uuid:d692bf96-ccf8-47bf-b246-1bbedcce60e5.
Full textTregloan-Reed, Jeremy. "Starspot properties and photometric parameters of transiting planets and their host stars." Thesis, Keele University, 2014. http://eprints.keele.ac.uk/1335/.
Full textChilders, Joseph M. "A search for transiting exoplanets in eclipsing binary stars." Virtual Press, 2008. http://liblink.bsu.edu/uhtbin/catkey/1398708.
Full textDepartment of Physics and Astronomy
Burke, Christopher J. "Survey for transiting extrasolar planets in stellar systems stellar and planetary content of the Open Cluster NGC 1245 /." Columbus, Ohio : Ohio State University, 2005. http://rave.ohiolink.edu/etdc/view?acc%5Fnum=osu1132168623.
Full textChadney, J. M., T. T. Koskinen, M. Galand, Y. C. Unruh, and J. Sanz-Forcada. "Effect of stellar flares on the upper atmospheres of HD 189733b and HD 209458b." EDP SCIENCES S A, 2017. http://hdl.handle.net/10150/626411.
Full textHood, Ben Andrew Ashcom. "Extrasolar planet search and characterisation." Thesis, St Andrews, 2007. http://hdl.handle.net/10023/359.
Full textMiller, Veronica Ruth. "A Search for Transiting Extrasolar Planets and Variable Stars in the Galactic Plane." Thesis, University of Canterbury. Physics and Astronomy, 2009. http://hdl.handle.net/10092/2858.
Full textBrown, David John Alexander. "The effects of tidal interactions on the properties and evolution of hot-Jupiter planetary systems." Thesis, University of St Andrews, 2013. http://hdl.handle.net/10023/4181.
Full textMulders, Gijs D., Ilaria Pascucci, Dániel Apai, Antonio Frasca, and Joanna Molenda-Żakowicz. "A SUPER-SOLAR METALLICITY FOR STARS WITH HOT ROCKY EXOPLANETS." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/622435.
Full textNuñez, P. D., N. J. Scott, B. Mennesson, O. Absil, J. C. Augereau, G. Bryden, Brummelaar T. ten, et al. "A near-infrared interferometric survey of debris-disc stars." EDP SCIENCES S A, 2017. http://hdl.handle.net/10150/626407.
Full textTeske, Johanna Kavanagh. "Connecting the Dots: Investigating Planet Formation and Composition Through Observations of Carbon and Oxygen Species in Stars, Disks, and Planets." Diss., The University of Arizona, 2014. http://hdl.handle.net/10150/318831.
Full textFossati, L., S. E. Marcelja, D. Staab, P. E. Cubillos, K. France, C. A. Haswell, S. Ingrassia, et al. "The effect of ISM absorption on stellar activity measurements and its relevance for exoplanet studies." EDP SCIENCES S A, 2017. http://hdl.handle.net/10150/624504.
Full textMatheus, Thiago. "Seleção de candidatos a sistemas planetários jovens." Universidade de São Paulo, 2010. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-14072010-211459/.
Full textCurrent models of planetary formation suggest that the giant gaseous planets are formed in time scales of ~ 10 Myr, less than the rocky ones, in time scales of ~ 30 Myr (Zuckerman & Song 2004). A simple test of these models of formation it would look for planets around young stars of various ages: in younger systems it should not detect terrestrial objects, which only appear around stars relatively older. CoRoT and Kepler satellites, which are at full system of observations, have been discovering exoplanets by the method of transits, being able to detect Earth-size bodies. The goal of this work is to select young planetary systems of various ages to be observed by the two satellites, in order to test the time scales of formation of rocky and gaseous planets. To achieve this goal it was necessary to understand how age can be estimated for a group of stars (open cluster or association), using, for example, data on chemical abundances of lithium objects. This is possible because of the ease of lithium to be destroyed in the pre-main sequence, at temperatures above 2,5 10^6 K. A sample survey of the abundance of lithium as a function of temperature for stars belonging to a group, generates a lithium depletion pattern, which creates a qualitatively model (da Silva et al. 2009) to obtain ages of star associations. For the purpose of this study was reached, the databases of objects in youth associations with well-determined ages from (Torres et al. 2008) was used, as well, the catalog DAML from (Dias et al. 2002) of open clusters. The selection of data for each satellite has produced quite different results. For CoRoT, the analysis of the database of associations returned results with a association in the galactic center and another with ~ 70 Myr in the anti-Galactic center, on the other hand, in the field of Kepler did not find young objects that would enable meet the goals of this work.. In the analysis of DAML catalog of open clusters have emerged many candidates targeted for observations. For the CoRoT was concluded that the clusters NGC 2244 of 7,87 Myr, NGC 2264 of 8,99 Myr, Collinder 107 of 10 Myr, Collinder 96 of 10,74 Myr, and NGC 2302 of 12,02 Myr contain targets where should be found only gas giant planets in the early stage and/or end of formation, in accordance with Chapter 1. The relatively older clusters, where they must be found rocky and gaseous planets are: NGC 6755 of 52,36 Myr, Basel 1 of 78,16 Myr, NGC 6694 of 85,31 Myr, NGC 2186 of 54,70 Myr, NGC 2422 of 72,61 Myr e Bochum 3 de 77,62 Myr. Therefore the step of selecting targets to be observed by the CoRoT was made, and thus, any observational results serve as a test for the timescales of planet formation proposed in the current models. For Kepler, it did not find any member of young cluster observed in its field of vision and its range of magnitudes.
Cauley, P. Wilson, Seth Redfield, Adam G. Jensen, and Travis Barman. "VARIATION IN THE PRE-TRANSIT BALMER LINE SIGNAL AROUND THE HOT JUPITER HD 189733B." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621234.
Full textLlama, Joseph. "Things that go bump in the light : an investigation into the effects of stellar activity on extrasolar planets." Thesis, University of St Andrews, 2014. http://hdl.handle.net/10023/4907.
Full textBaumann, Patrick. "The chemical composition of solar-type stars and its impact on the presence of planets." Diss., Ludwig-Maximilians-Universität München, 2013. http://nbn-resolving.de/urn:nbn:de:bvb:19-156280.
Full textFossati, L., T. Koskinen, K. France, P. E. Cubillos, C. A. Haswell, A. F. Lanza, and I. Pillitteri. "Suppressed Far-UV Stellar Activity and Low Planetary Mass Loss in the WASP-18 System." IOP PUBLISHING LTD, 2018. http://hdl.handle.net/10150/627089.
Full textRicci, L., P. Cazzoletti, I. Czekala, S. M. Andrews, D. Wilner, L. Szűcs, G. Lodato, et al. "ALMA Observations of the Young Substellar Binary System 2M1207." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624920.
Full textStevens, Daniel Joseph. "Discovery and Characterization of Hot Stars and their Cool, Transiting Companions." The Ohio State University, 2018. http://rave.ohiolink.edu/etdc/view?acc_num=osu1531147521265881.
Full textLaws, Christopher S. "The chemically peculiar nature of stars with planets : searching for signatures of accretion in stellar photospheres /." Thesis, Connect to this title online; UW restricted, 2004. http://hdl.handle.net/1773/5430.
Full textKastner, Joel H., David A. Principe, Kristina Punzi, Beate Stelzer, Uma Gorti, Ilaria Pascucci, and Costanza Argiroffi. "M STARS IN THE TW HYA ASSOCIATION: STELLAR X-RAYS AND DISK DISSIPATION." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621232.
Full textFeng, Y. Katherina, Michael R. Line, Jonathan J. Fortney, Kevin B. Stevenson, Jacob Bean, Laura Kreidberg, and Vivien Parmentier. "THE IMPACT OF NON-UNIFORM THERMAL STRUCTURE ON THE INTERPRETATION OF EXOPLANET EMISSION SPECTRA." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621967.
Full textSee, Wyke Chun Victor. "Stellar magnetism and activity : from stellar interiors to orbiting exoplanets." Thesis, University of St Andrews, 2016. http://hdl.handle.net/10023/9602.
Full textNielsen, Eric L., Robert J. De Rosa, Jason Wang, Julien Rameau, Inseok Song, James R. Graham, Bruce Macintosh, et al. "DYNAMICAL MASS MEASUREMENT OF THE YOUNG SPECTROSCOPIC BINARY V343 NORMAE AaAb RESOLVED WITH THE GEMINI PLANET IMAGER." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/622436.
Full textWilson, Robert F., Johanna Teske, Steven R. Majewski, Katia Cunha, Verne Smith, Diogo Souto, Chad Bender, et al. "Elemental Abundances of Kepler Objects of Interest in APOGEE. I. Two Distinct Orbital Period Regimes Inferred from Host Star Iron Abundances." IOP PUBLISHING LTD, 2018. http://hdl.handle.net/10150/626528.
Full textKonopacky, Q. M., C. Marois, B. A. Macintosh, R. Galicher, T. S. Barman, S. A. Metchev, and B. Zuckerman. "ASTROMETRIC MONITORING OF THE HR 8799 PLANETS: ORBIT CONSTRAINTS FROM SELF-CONSISTENT MEASUREMENTS." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621227.
Full textRajan, Abhijith, Julien Rameau, Robert J. De Rosa, Mark S. Marley, James R. Graham, Bruce Macintosh, Christian Marois, et al. "Characterizing 51 Eri b from 1 to 5 mu m: A Partly Cloudy Exoplanet." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624674.
Full textChristiansen, Jessie L., Andrew Vanderburg, Jennifer Burt, B. J. Fulton, Konstantin Batygin, Björn Benneke, John M. Brewer, et al. "Three’s Company: An Additional Non-transiting Super-Earth in the Bright HD 3167 System, and Masses for All Three Planets." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/625817.
Full textSchlawin, E., T. Herter, M. Zhao, J. K. Teske, and H. Chen. "REDUCED ACTIVITY AND LARGE PARTICLES FROM THE DISINTEGRATING PLANET CANDIDATE KIC 12557548b." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621392.
Full textGodolt, Mareike [Verfasser], and Heike [Akademischer Betreuer] Rauer. "3D climate modeling of Earth-like extrasolar planets orbiting different types of central stars / Mareike Godolt. Betreuer: Heike Rauer." Berlin : Universitätsbibliothek der Technischen Universität Berlin, 2012. http://d-nb.info/1028912862/34.
Full textMohler-Fischer, Maren [Verfasser], and Thomas [Akademischer Betreuer] Henning. "Search for extrasolar planets around young stars in the presence of stellar activity / Maren Mohler-Fischer ; Betreuer: Thomas Henning." Heidelberg : Universitätsbibliothek Heidelberg, 2013. http://d-nb.info/1177382733/34.
Full textSabotta, Silvia [Verfasser], Artie [Gutachter] Hatzes, Konstanze [Gutachter] Zwintz, and Magali [Gutachter] Deleuil. "The frequency of planets around A- and M-type stars / Silvia Sabotta ; Gutachter: Artie Hatzes, Konstanze Zwintz, Magali Deleuil." Jena : Friedrich-Schiller-Universität Jena, 2021. http://nbn-resolving.de/urn:nbn:de:gbv:27-dbt-20210818-100712-001.
Full textDeshpande, Rohit. "Search for gas giants around late-M dwarfs." Doctoral diss., University of Central Florida, 2010. http://digital.library.ucf.edu/cdm/ref/collection/ETD/id/4640.
Full textID: 029094443; System requirements: World Wide Web browser and PDF reader.; Mode of access: World Wide Web.; Thesis (Ph.D.)--University of Central Florida, 2010.; Includes bibliographical references (p. 224-246).
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