Search results for "52"
showing 10 items of 1043 documents
New Insights into Galaxy Clusters: from Simulations to Observations
2011
The work carried out during this Thesis is framed within the field of Numerical Cosmology and focused on several broad lines intimately related which deal with the theoretical and numerical study of galaxy clusters: (i) the halo-finding problem, (ii) new improvements in cosmological simulations, and (iii) the formation and evolution of galaxy clusters. In spite of the achievements reached by Computational Cosmology in the last years, present-day hydrodynamics/N-body simulations still present important discrepancies with the observations, especially in the inner regions of massive galaxy clusters. Among these discrepancies we can cite, for instance, the breaking up of the self-similar scalin…
Asteroseismology and mass loss in Be stars. Study with CoRoT
2010
The interiors of the stars are among the most difficult parts of the Universe to observe. Essentially, asteroseismology tries to make use of the oscillations to prove the stellar interiors, which are not directly observable. The basic principles of asteroseismology are, to a certain extent, similar to those developed and employed by Earth seismologists. Asteroseismology relies on advanced mathematical descriptions of oscillations in a three-dimensional body and numerical modeling. It is therefore a prominent example of interdisciplinary science. The general aim of this work is the study of Be stars with the CoRoT space mission. Classical Be stars are B-type stars that exhibit line emission …
Magnetohidrodinámica relativista numérica: Aplicaciones en relatividad especial y general.
2008
En muchos escenarios astrof´ýsicos (acreci´on de discos, chorros, colapso estelar,etc) podemos encontrar que los campos magn´eticos juegan un papel crucialen uni´on a velocidades relativistas y/o fuertes campos gravitatorios. En muchosde estos escenarios se cumplen las condiciones necesarias para poder serdescritos en terminos de la magnetohidrodin´amica relativista ideal (RMHD).El objetivo principal de esta Tesis ha sido el desarrollo de un c´odigo capazde resolver las ecuaciones de la magnetohidrodin´amica en relatividad especialy general basado en t´ecnicas de alta resoluci´on de captura de choques (HRSC).Este tipo de t´ecnicas explota el car´acter conservativo e hiperb´olico del sistema…
Models cosmològics inhomogenis conformement plans
2002
En aquest treball parlem de models cosmològics conformement plans en dos sentits, aquells que tenen una mètrica associada que és conformement plana en el sentit de mètrica d'espai-temps 4-dimensional, i aquells que tenen associades unes seccions espacials conformement planes en el sentit de mètriques 3-dimensionals. Ambdós sentits de mètriques conformement planes simplifiquen considerablement el tractament de les equacions d'Einstein al restringir-nos a espai-temps els quals tenen un únic grau de llibertat representat per una funció arbitrària de les coordenades. Als espais-temps conformement plans aquesta funció està representada pel factor de conformitat corresponent; mentre que als espai…
On the FON astroplate project accomplishment
2019
The plan for a photographic survey of the northern sky (FON) was proposed at the Golosiiv observatory (Main Astronomical Observatory, NAS of Ukraine, Kyiv, Ukraine) in the late 1970-ies [Pakuliak et al., 2016; Vavilova, 2016; Vavilova et al., 2017]. The last compilation of the final catalog of objects involves 5,700 digitized astroplates of four observatories: MAO NAS of Ukraine (Kyiv, Ukraine) [Andruk et al., 2016], Kitab Astronomical Observatory (Tashkent, Uzbekistan) [Yuldoshev et al., 2017], Gissar Astronomical Observatory (Dushanbe, Tajikistan) [Mullo-Abdolov et al., 2017, 2018], and the observatory in Baldone (Latvia) [Eglitis, 2017]. The consolidated catalog of positions and B-magnit…
"Table 10" of "First measurement of quarkonium polarization in nuclear collisions at the LHC"
2021
$\Upsilon(1{\rm S})$ polarization parameters in the helicity and Collins-Soper reference frames measured in Pb--Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ TeV in the rapidity interval $2.5
"Table 9" of "First measurement of quarkonium polarization in nuclear collisions at the LHC"
2021
$\Upsilon(1{\rm S})$ polarization parameters in the helicity and Collins-Soper reference frames measured in Pb--Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ TeV in the rapidity interval $2.5
"Table 11" of "First measurement of quarkonium polarization in nuclear collisions at the LHC"
2021
$\Upsilon(1{\rm S})$ polarization parameters in the helicity and Collins-Soper reference frames measured in Pb--Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ TeV in the rapidity interval $2.5
CCDC 1950443: Experimental Crystal Structure Determination
2021
Related Article: Liu-Pan Yang, Li Zhang, Mao Quan, Jas S. Ward, Yan-Long Ma, Hang Zhou, Kari Rissanen, Wei Jiang|2020|Nat.Commun.|11|2740|doi:10.1038/s41467-020-16534-9
CCDC 1913148: Experimental Crystal Structure Determination
2019
Related Article: Hongxin Chai, Zhi-Sheng Pan, Liu-Pan Yang, Shan He, Fangfang Pan, Kari Rissanen, Wei Jiang|2019|Chem.Commun.|55|7768|doi:10.1039/C9CC03341F