Tesis sobre el tema "Tully-Fisher relation"
Crea una cita precisa en los estilos APA, MLA, Chicago, Harvard y otros
Consulte los 19 mejores tesis para su investigación sobre el tema "Tully-Fisher relation".
Junto a cada fuente en la lista de referencias hay un botón "Agregar a la bibliografía". Pulsa este botón, y generaremos automáticamente la referencia bibliográfica para la obra elegida en el estilo de cita que necesites: APA, MLA, Harvard, Vancouver, Chicago, etc.
También puede descargar el texto completo de la publicación académica en formato pdf y leer en línea su resumen siempre que esté disponible en los metadatos.
Explore tesis sobre una amplia variedad de disciplinas y organice su bibliografía correctamente.
Young, Paul. "The Tully-Fisher relation in nearby clusters". Thesis, Durham University, 1996. http://etheses.dur.ac.uk/5097/.
Texto completoBarden, Marco. "The Evolution of the Tully-Fisher Relation at Redshift z~1". Diss., lmu, 2004. http://nbn-resolving.de/urn:nbn:de:bvb:19-29114.
Texto completoBonhomme, Nicolas. "Cosmographie de l’univers local : analyse de données pour la relation de Tully-Fisher". Thesis, Lyon 1, 2010. http://www.theses.fr/2010LYO10048/document.
Texto completoThis phD thesis is part of the COSFLOS’project. Its goal is to understand the galaxy structure evolution in the local universe. For this purpose, we make use of the Tully-Fisher relation in order to measure the distances for galaxies within 80 Mpc. My research area in the project is to collect, measure and analyze the data needed for the Luminosity LineWidth (LLW). This relation is a direct link between intrinsic luminosity of a spiral galaxy and its maximal gas rotation velocity. The best way to compute this velocity is to measure HI linewidth. Including my new observations and measurements, the current extragalactic database EDD contains 15 411 HI profiles. To obtain the apparent magnitude needed for the distances, I improve the ARCHANGEL software, implementing new displays. We took a great care to a special parameter : the inclination of observed galaxy. Finally, I present the Antlia cluster, one of the cluster I use to calibrate the slope of the LLW. I start with the candidates selection, then with observations to finally obtain the distances for the calibration
Bonhomme, Nicolas. "Cosmographie de l'univers local : analyse de données pour la relation de Tully-Fisher". Phd thesis, Université Claude Bernard - Lyon I, 2010. http://tel.archives-ouvertes.fr/tel-00522062.
Texto completoTiley, Alfred. "Probing the evolution of galaxies since z ~ 1 with the Tully-Fisher relation". Thesis, University of Oxford, 2016. https://ora.ox.ac.uk/objects/uuid:1169c5e2-5962-47a4-8c9f-f58fcf93bf68.
Texto completoHan, Mingsheng Mould Jeremy Mould Jeremy. "The I-band Tully-Fisher relation and large-scale motions in the universe /". Diss., Pasadena, Calif. : California Institute of Technology, 1991. http://resolver.caltech.edu/CaltechETD:etd-06222007-113504.
Texto completoTheureau, Gilles. "L'échelle des distances extragalactiques : la relation Tully-Fisher et la constante de Hubble Ho". Observatoire de Paris (1667-....), 1997. https://hal.science/tel-02153817.
Texto completoThis thesis presents an exhaustive study of the Tully-Fisher (TF) relation on the basis of the largest available sample of field spiral galaxies. This co-called KLUN sample, containing 6620 galaxies from type Sa to Sdm, has been collected from LEDA data base and studied in detail for completeness and homogeneity. It allows to investigate the various aspects of the B-band TF relation both with diameter and magnitude, direct or inverse relations. I report on an advanced version of the normalized distance method (Bottinelli et al. 1986), now taking into account all the variations of the Malmquist bias the observable parameters space. Its validation in statistical terms leads to work out a new bias correction method allowing to study the peculiar velocity field up to 200 Mpc. In addition, I show that introducing additional parameters such as morphological type or mean surface brightness reduces the TF intrinsic scatter and allows to extend the unbiased distance range. Then, a statistically reliable value of the Hubble constant Ho is obtained from an unbiased subsample of 600 field galaxies (z ≤ 0. 02), in perfect agreement with the results derived at greater distance from type Ia supernovae (up to z=0. 1). This value H0=55 ± 5 km s-1 Mpc-1 depends only on the primary calibration, i. E. Cepheid distances. I give an independent estimate of the Local Group infall toward Virgo (Vgl=200 ± 300 km s-1), confirm the existence of a Local Anomaly of the velocity field limited too Leo spur and Sculptor cloud, and show evidence for an infall pattern (front and back side infall) in the vinicity of some great mass concentrations such as Hydra or Perseus-Pisces clusters. The prominent bulk flow expected in the direction of the Great Attractor is not confirmed
Iodice, Enrichetta. "Formation Scenarios for Polar Ring Galaxies". Doctoral thesis, SISSA, 2001. http://hdl.handle.net/20.500.11767/4321.
Texto completoSoliman, Khaled Said Ahmed. "Peculiar flow fields in the zone of avoidance from the near-infrared Tully-Fisher relation". Doctoral thesis, University of Cape Town, 2017. http://hdl.handle.net/11427/25463.
Texto completoPizagno, James Lawrence II. "The Tully-Fisher Relation, its residuals, and a comparison to theoretical predictions for a broadly selected sample of galaxies". The Ohio State University, 2006. http://rave.ohiolink.edu/etdc/view?acc_num=osu1154980670.
Texto completoAffadi, Ikechukwu Patrick. "A new method of mapping cosmic flow fields : evaluating the sustainability of the infrared bands Tully-Fisher relation for ZoA work". Master's thesis, University of Cape Town, 2016. http://hdl.handle.net/11427/20813.
Texto completoYegorova, Iryna. "Dark matter in spiral galaxies". Doctoral thesis, SISSA, 2007. http://hdl.handle.net/20.500.11767/4184.
Texto completoPuech, Mathieu. "Contraintes apportées par la spectroscopie intégrale de champ à la formation et à l'évolution des galaxies". Phd thesis, Université Paris-Diderot - Paris VII, 2006. http://tel.archives-ouvertes.fr/tel-00012037.
Texto completoTorres, Flores Sergio Patricio. "Etude de la cinématique des galaxies dans les groupes compacts". Aix-Marseille 1, 2010. http://theses.univ-amu.fr.lama.univ-amu.fr/2010AIX11050.pdf.
Texto completoThis thesis presents results on the kinematics, scaling relations and structures of 48 galaxies in 22 compact groups. For 35 galaxies in 12 compact groups, velocity fields, monochromatic maps (derived from Hα observations) and velocity dispersion maps are presented for the first time. By using these data, it was possible to determine the kinematic and morphological parameters, the rotation curves and to derive the Tully-Fisher relation for the galaxies in dense environments. By using the maximum rotational velocity for each galaxy (derived from its rotation curve) and its optical and near-infrared luminosity and mass, the different Tully-Fisher relations for galaxies in compact groups were derived. Comparing these results with the results displayed by galaxies in less dense environments, it was found that galaxies in compact groups agrees with the Tully-Fisher relation defined by non-interacting galaxies. However, some of the low-mass galaxies are off the Tully-Fisher relation, having too high luminosities for their maximum rotational velocities. This scenario can be explained by a burst of star formation and/or by nuclear activity. We conclude that the maximum rotational velocities of compact groups galaxies are not affected during galaxy-galaxy interactions which implies that there is no significant mass stripping in galaxies of compact groups inside their optical radius. The mass distribution of galaxies in compact groups indicates that the rotation curves of these galaxies are highly asymmetric. The asymmetry could be produced by interactions between galaxies. These interactions, besides affecting the shape of the rotation curve, can eject some neutral gas from the disk of the interacting galaxies into the intragroup medium. By using ultraviolet data, we find several young star-forming regions in the intragroup medium of compact groups. It is still an open question wether these young stellar systems can survive and become new members of the group or if they will fall back onto their parent galaxies
Gurovich, Sebastian. "An observational study of the Baryonic Tully-Fisher relation". Phd thesis, 2006. http://hdl.handle.net/1885/149697.
Texto completoGoetz, Andrew Stewart. "The Einstein-Klein-Gordon Equations, Wave Dark Matter, and the Tully-Fisher Relation". Diss., 2015. http://hdl.handle.net/10161/9927.
Texto completoWe examine the Einstein equation coupled to the Klein-Gordon equation for a complex-valued scalar field. These two equations together are known as the Einstein-Klein-Gordon system. In the low-field, non-relativistic limit, the Einstein-Klein-Gordon system reduces to the Poisson-Schrödinger system. We describe the simplest solutions of these systems in spherical symmetry, the spherically symmetric static states, and some scaling properties they obey. We also describe some approximate analytic solutions for these states.
The EKG system underlies a theory of wave dark matter, also known as scalar field dark matter (SFDM), boson star dark matter, and Bose-Einstein condensate (BEC) dark matter. We discuss a possible connection between the theory of wave dark matter and the baryonic Tully-Fisher relation, which is a scaling relation observed to hold for disk galaxies in the universe across many decades in mass. We show how fixing boundary conditions at the edge of the spherically symmetric static states implies Tully-Fisher-like relations for the states. We also catalog other ``scaling conditions'' one can impose on the static states and show that they do not lead to Tully-Fisher-like relations--barring one exception which is already known and which has nothing to do with the specifics of wave dark matter.
Dissertation
Han, Mingsheng. "The I-band Tully-Fisher relation and large-scale motions in the universe". Thesis, 1991. https://thesis.library.caltech.edu/2690/1/Han_m_1991.pdf.
Texto completoBarden, Marco [Verfasser]. "The evolution of the Tully-Fisher relation at redshift z ̃1 / vorgelegt von Marco Barden". 2004. http://d-nb.info/973265752/34.
Texto completoHALL, MELANIE. "An Investigation of Sloan Digital Sky Survey Data and Multi-Band Scaling Relations of Spiral Galaxies". Thesis, 2010. http://hdl.handle.net/1974/6049.
Texto completoThesis (Master, Physics, Engineering Physics and Astronomy) -- Queen's University, 2010-09-17 16:23:20.649