Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Paul Ledoux"'
Autor:
Paul Ledoux, Allen Cole
Big dreams, risk takers, a sexy sports car: what more could you want in a musical? With catchy 1970's pop and funk inspired tunes, The Bricklin takes audiences on a fantastical and wild ride through politics, business antics, and controversy… as it
Autor:
Paul Ledoux, D.O. Gough
Publikováno v:
International Astronomical Union Colloquium. 185:37-57
Much of our knowledge of the hydrodynamics of stellar oscillations is summarized in the now-classical article by Ledoux & Walraven in volume 51 of the Handbuch der Physik. It is from that article that I, and many others, first learned the subject. Mo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bd629dafd0281bd850686d1e5a368a58
https://doi.org/10.1017/s0252921100015530
https://doi.org/10.1017/s0252921100015530
Autor:
Paul Ledoux
Publikováno v:
Problems of Stellar Convection ISBN: 9783540085324
The linear dynamical instability at the origin of convection in stars is reviewed and shown to depend essentially on the sign of $$A = \frac{1}{\rho }\frac{{d\rho }}{{dr}} - \frac{1}{{\Gamma _1 p}}\frac{{dp}}{{dr}}$$ which is the usual argument of co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::877c273a3399af0faa592eca3b9d7a40
https://doi.org/10.1007/3-540-08532-7_34
https://doi.org/10.1007/3-540-08532-7_34
Autor:
Paul Ledoux
Publikováno v:
Highlights of Astronomy. 5:433-436
Aside from violent phenomena, regular forms of motions originate often in instabilities and the linear theory with terms ∞ exp (st) yields already significant information. The system, here a spherical star, will be the seat of an instability if R (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::15d6632f46cc0b5524ab47a4cf4f3ea2
https://doi.org/10.1017/s1539299600004172
https://doi.org/10.1017/s1539299600004172
Autor:
Paul Ledoux, H. Robe
Publikováno v:
Bulletin de la Classe des sciences. 61:198-209
— The non radial oscillations of the standard model are studied numerically for values of the degree l, of the spherical harmonics ranging from l = 2 to l = 50 in the case of the g modes and l = 2 to 200 in the case of the ƒ and p modes. It is fou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0ab4a7d63809aa3e35ad2edf068299e0
https://doi.org/10.3406/barb.1975.57908
https://doi.org/10.3406/barb.1975.57908
Autor:
Paul Ledoux
Publikováno v:
Symposium - International Astronomical Union. 3:186-199
The most immediate purpose of the study of stellar stability is to discover the sources of incipient instability which must be responsible for the observed variability of a great number of stars.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b28ae3471d54ce18334c0a605433d992
https://doi.org/10.1017/s0074180900018799
https://doi.org/10.1017/s0074180900018799
Autor:
Paul Ledoux
Publikováno v:
Highlights of Astronomy. 1:12-32
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b654d68beed6d91a5efc74f4be99ce28
https://doi.org/10.1017/s1539299600000988
https://doi.org/10.1017/s1539299600000988
Autor:
Paul Ledoux
Publikováno v:
Périodiques Scientifiques en Édition Électronique.
After some general remarks on secular stability and stellar evolution, the problem is discussed by means of the small perturbation method. Apart from recovering very simply the usual criteria of dynamical and vibrational stability, this leads, for se
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ef57247de970908c7405406711ca4790
https://www.persee.fr/doc/barb_0001-4141_1960_num_46_1_67940
https://www.persee.fr/doc/barb_0001-4141_1960_num_46_1_67940