Les variations de cycle à cycle de la Céphéide l Car
Références
[1] Kervella, P. and Nardetto, N. and Bersier, D.and Mourard, D. and Coudé du Foresto, V. 2004, 416, 941-953, http://cdsads.u-strasbg.fr/abs/2004A%26A...416..941K [Provided by the SAO/NASA Astrophysics Data System]
[2] Leavitt, H. S. 1908, Annals of Harvard College Observatory, 60, 87, http://cdsads.u-strasbg.fr/abs/1908AnHar..60...87L [Provided by the SAO/NASA Astrophysics Data System]
[3] Leavitt, H. S. 1912, Periods of 25 Variable Stars in the Small Magellanic Cloud, 173, 1-3, http://cdsads.u-strasbg.fr/abs/1912HarCi.173....1L [Provided by the SAO/NASA Astrophysics Data System]
[4] Shapley, H. 1918, Studies based on the colors and magnitudes in stellar clusters. VII. Thedistances, distribution in space, and dimensions of 69 globular clusters, 48, http://cdsads.u-strasbg.fr/abs/1918ApJ....48..154S [Provided by the SAO/NASA Astrophysics Data System]
[5] Hubble, E. 1929, A Relation between Distance and Radial Velocity among Extra-Galactic Nebulae, 15, 168-173, http://cdsads.u-strasbg.fr/abs/1929PNAS...15..168H [Provided by the SAO/NASA Astrophysics Data System]
[6] Kervella, P. and Bersier, D. and Mourard, D. and Nardetto, N. and Coudé du Foresto, V. 2004, 423, 327-333, http://cdsads.u-strasbg.fr/abs/2004A%26A...423..327K Provided by the SAO/NASA Astrophysics Data System]
[7] Nardetto, N. and Fokin, A. and Mourard, D. and Mathias, P. and Kervella, P. and Bersier, D. 2004, Self consistent modelling of the projection factor for interferometric distance determination, 428, 131-137, http://cdsads.u-strasbg.fr/abs/2004A%26A...428..131N [Provided by the SAO/NASA Astrophysics Data System]
[8] Anderson, R. I. 2016, Discovery of Cycle-to-cycle Modulated Spectral Line Variability and Velocity Gradients in Long-period Cepheids, 463, 1707-1723, http://cdsads.u-strasbg.fr/abs/2016MNRAS.463.1707A [Provided by the SAO/NASA Astrophysics Data System]
[9] Storm, J. and Gieren, W. and Fouqué, P. and Barnes, T. G. and Pietrzynski, G. and Nardetto, N. and Weber, M. and Granzer, T. and Strassmeier, K. G. 2011, Calibrating the Cepheid period-luminosity relation from the infrared surface brigthness technique. I. The p-factor, the Milky Way relations, and a universal K-band relation, 534, http://cdsads.u-strasbg.fr/abs/2011A%26A...534A..94S [Provided by the SAO/NASA Astrophysics Data System]
[10] Site de données astronomiques,
http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=l+car&submit=SIMBAD+search
[11] Nardetto N. 2005, La dynamique atmosphérique des
Céphéides et l'étalonnage des distances dans l'Univers,
https://www.theses.fr/103220917
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[13] Kervella, P. and Nardetto, N. and Bersier, D. and Mourard, D. and Coudé du Foreste, V., 2004, Cepheid distances from infrared long-baseline interferometry. I. VINCI/VLTI observations of seven Galactic Cepheids, 416, 941-953, http://cdsads.u-strasbg.fr/abs/2004A%26A...416..941K [Provided by the SAO/NASA Astrophysics Data System]
[14] Nardetto, N. and Mourard, D. and Mathias, P. and Fokin, A. and Gillet, D., 2007, High-resolution spectroscopy for Cepheids distance determination. II. A period-projection factor relation, 471, 661-669,http://cdsads.u-strasbg.fr/abs/2007A%26A...471..661N [Provided by the SAO/NASA Astrophysics Data System]
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Remerciements
Je remercie tout d'abord l'Observatoire de la Côte d'Azur de m'avoir accueillie pour mon projet tuteuré en laboratoire.
Je remercie aussi toutes les personnes de l'Observatoire qui ont su m'aider sur des points particuliers, à divers moments.
Au terme de ma licence, j'aimerais également adresser mes remerciements à l'ensemble des professeurs de Physique-Chimie de l'Université Nice - Sophia Antipolis.
Je remercie enfin sincèrement Nicolas Nardetto pour son aide, sa disponibilité et pour les connaissances qu'il m'a apportées dans la découverte de l'astrophysique, domaine que je méconnaissais jusque là et qui m'a finalement beaucoup plu.