Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Kerber, Leandro O."'
Autor:
de Souza, Gabriel Fabiano, Westera, Pieter, Almeida-Fernandes, Felipe, Limberg, Guilherme, Dias, Bruno, Hernandez-Jimenez, José A., Herpich, Fábio R., Kerber, Leandro O., Machado-Pereira, Eduardo, Perottoni, Hélio D., Guerço, Rafael, Li, Liana, Sampedro, Laura, Kanaan, Antonio, Ribeiro, Tiago, Schoenell, William, de Oliveira, Claudia Mendes
The Magellanic Clouds are the most massive and closest satellite galaxies of the Milky Way, with stars covering ages from a few Myr up to 13 Gyr. This makes them important for validating integrated light methods to study stellar populations and star-
Externí odkaz:
http://arxiv.org/abs/2310.15158
Autor:
Amores, Eduardo B., Jesus, Ricardo M., Moitinho, Andre, Arsenijevic, Vladan, Levenhagen, Ronaldo S., Marshall, Douglas J., Kerber, Leandro O., Kunzel, Roseli, Moura, Rodrigo A.
Estimates of interstellar extinction are essential in a broad range of astronomical research. In the last decades, several maps and models of the large scale interstellar extinction in the Galaxy have been published. However, these maps and models ha
Externí odkaz:
http://arxiv.org/abs/2108.00561
Autor:
Souza, Stefano O., Kerber, Leandro O., Barbuy, Beatriz, Pérez-Villegas, Angeles, Oliveira, Raphael A. P., Nardiello, Domenico
The Bayesian isochrone fitting using the Markov chain Monte Carlo algorithm is applied, to derive the probability distribution of the parameters age, metallicity, reddening, and absolute distance modulus. We introduce the \texttt{SIRIUS} code by mean
Externí odkaz:
http://arxiv.org/abs/2001.02697
Akademický článek
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Autor:
Dias, Bruno M. S., Kerber, Leandro O., Santiago, Basílio X., Barbuy, Beatriz, Balbinot, Eduardo
The Magellanic Clouds (MCs) present a rich system of stellar clusters that can be used to probe the dynamical and chemical evolution of these neighboring and interacting irregular galaxies. In particular, these stellar clusters (SCs) present combinat
Externí odkaz:
http://arxiv.org/abs/0809.3775
We investigate the properties of two stellar concentrations in a low-absorption disk zone in Centaurus, located respectively at $\ell=306.47^{\circ}$, $b=-0.61 ^{\circ}$, and $\ell=307.01^{\circ}$, $b=-0.74 ^{\circ}$. The present analysis is based mo
Externí odkaz:
http://arxiv.org/abs/astro-ph/0504029
Akademický článek
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Autor:
Amôres, Eduardo B, Jesus, Ricardo M, Moitinho, André, Arsenijevic, Vladan, Levenhagen, Ronaldo S, Marshall, Douglas J, Kerber, Leandro O, Künzel, Roseli, Moura, Rodrigo A
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Dec2021, Vol. 508 Issue 2, p1788-1797, 10p
Autor:
Kerber, Leandro O.1,2, Santiago, Basílio X.3
Publikováno v:
Proceedings of the International Astronomical Union. 07/02/2008, Vol. 4 Issue S256, p391-396. 6p.