Zobrazeno 1 - 5
of 5
pro vyhledávání: '"D. B. de Castro"'
Publikováno v:
The international journal of tuberculosis and lung disease : the official journal of the International Union against Tuberculosis and Lung Disease. 22(2)
Setting Brazil ranks eighteenth worldwide in annual numbers of new tuberculosis (TB) cases. The municipality of Manaus, Amazonas State, has the highest incidence of TB in Brazil. Objective To evaluate the quality of TB epidemiological surveillance, a
Autor:
E. Jilinski, J. V. Sales Silva, Fernando Roig, D. B. de Castro, Natalia A. Drake, C. B. Pereira, C. Chavero
In this paper we present an homogeneous analysis of photospheric abundances based on high-resolution spectroscopy of a sample of 182 barium stars and candidates. We determined atmospheric parameters, spectroscopic distances, stellar masses, ages, lum
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6e7deeb50b1b8f343c390a6766e1f9b7
http://arxiv.org/abs/1604.03031
http://arxiv.org/abs/1604.03031
Autor:
Amanda I. Karakas, Sergio Cristallo, Marco Pignatari, Valentina D'Orazi, B. Cseh, D. B. de Castro, Emese Plachy, Claudio B. Pereira, László Molnár, Maria Lugaro, Róbert Szabó
Publikováno v:
Astronomy & Astrophysics. 620:A146
Context. Barium (Ba) stars are dwarf and giant stars enriched in elements heavier than iron produced by the slow neutron-capture process (s process). They belong to binary systems where the primary star evolved through the asymptotic giant branch (AG
Publikováno v:
The Astronomical Journal. 146:39
Open clusters are very useful examples to explain the constraint of the nucleosynthesis process with the luminosities of stars because the distances of the clusters are better known than those of field stars. We carried out a detailed spectroscopic a
Autor:
Fernando Roig, V. G. Ortega, C. Chavero, D. B. de Castro, C. B. Pereira, Natalia A. Drake, E. Jilinski
Publikováno v:
Astronomy & Astrophysics. 543:A58
High-velocity halo stars provide important information about the properties of the extreme Galactic halo. The study of unbound and bound Population II stars permits us to better estimate the mass of the halo.} {We carried out a detailed spectroscopic