Zobrazeno 1 - 10
of 80
pro vyhledávání: '"Irapuan Rodrigues"'
Autor:
Vinícius Daniel Reis de Castro, Francisco C. R. Fernandes, Lucas Antonio Caritá, Irapuan Rodrigues
Publikováno v:
Revista UniVap, Vol 29, Iss 63 (2023)
Este trabalho apresenta um estudo estatístico das capturas de meteoros da chuva Southern Delta-Aquariids (SDA). Os registros foram feitos pelas câmeras das estações de monitoramento de meteoros UVP1 e UVP2, da rede EXOSS, instaladas em São José
Externí odkaz:
https://doaj.org/article/370d31bb14d140cbbe7f3c0a6ccd8089
Publikováno v:
Revista UniVap, Vol 29, Iss 61 (2023)
As galáxias espirais normais possuem um núcleo, disco, bojo, halo e braços espirais. Esses sistemas despertam muita curiosidade, atração e questionamentos científicos e consequentemente, muitos estudos e técnicas são propostas para análise d
Externí odkaz:
https://doaj.org/article/2f1f5fb1e5c046748dc08fe63c73af37
Autor:
Faria Costa, Stella1 steefaria@gmail.com, de Oliveira Filho, Irapuan Rodrigues2 irapuan.rodrigues@gmail.com, Antonio Caritá, Lucas3 prof.carita@ifsp.edu.br
Publikováno v:
Revista UniVap. 2023, Vol. 29 Issue 61, p1-11. 11p.
Autor:
Felipe Alexandre da Silva, Vinicius Daniel dos Reis de Castro, Marcos William da Silva Oliveira, Lucas Antonio Caritá, Irapuan Rodrigues, Francisco Carlos Rocha Fernandes
Publikováno v:
Asian Journal of Mathematics and Computer Research. 30:1-8
Determining the portion obscured by clouds in the night sky recorded in an image from a meteor monitoring station can be useful to help in the discussion and analysis of studies in this area. Thereby, this work presents a proposal to quantitatively m
Autor:
Bica, Eduardo, Dottori, Horacio, F., Irapuan Rodrigues de Oliveira, Ortolan, Sergio, Barbuy, Beatriz
The recent detection of a double Red Giant Branch in the optical color-magnitude diagram (CMD) of the bulge globular cluster HP1 (Ortolani et al. 1997), a more populated metal-poor steep one corresponding to the cluster itself, and another metal-rich
Externí odkaz:
http://arxiv.org/abs/astro-ph/9703166
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 501:3750-3766
We investigate the interaction effects in the stellar and gas kinematics, stellar population and ionized gas properties in the interacting galaxy pair AM1209-292, composed by NGC4105 and NGC4106. The data consist of long-slit spectra in the range of
Publikováno v:
Galaxies, Vol 5, Iss 4, p 101 (2017)
One of the algebraic potentials most commonly used to represent a galactic bar in the stellar orbits integration is the Ferrers potential. Some researchers may be inclined to implement a numerical differentiation for it in the motion or variational e
Externí odkaz:
https://doaj.org/article/9920eed6973548c29015808703fb42db
Publikováno v:
Revista Mexicana de Astronomía y Astrofísica. 55:321-335
This paper aims to verify the influence of the bar, its pattern speed (Ω_b) and its rate of growth on the stability of the orbits in gravitational potentials. We studied the nature of the orbits in potentials representing galaxies with growing bars
Autor:
L. J. de Melo de Azevedo, L. Katena, Antonio Kanaan, Paula Coelho, M. V. Costa-Duarte, F. Urrutia-Viscarra, A. Schnorr Müller, Irapuan Rodrigues, Erik V.R. de Lima, Angela Krabbe, David Alexander Kann, M. Vika, Carlos Gabriel Escudero, S. Alencar, Dennis Zaritsky, Nina S. T. Hirata, G. Damke, Fernando Roig, H. Farías, Leonardo A. Almeida, Anthony H. Gonzalez, D. Brito-Silva, Favio Raúl Faifer, F. Almeida-Fernandes, Luca Izzo, H. J. Rocha Pinto, O. L. Dors, W. A. Santos, M. Jaque Arancibia, Rafael M. Santucci, Pieter Westera, Yara L. Jaffé, Bruno Quint, Kanak Saha, R. S. Nemmen, Roberto K. Saito, L. A. Gutiérrez-Soto, Silvia Rossi, Leandro Alberto Sesto, Lilianne Mariko Izuti Nakazono, Ana L. Chies-Santos, L. Azanha, C. Labayru, Christina C. Thöne, William Schoenell, C. Lima-Dias, A. de Ugarte Postigo, S. S. Eikenberry, Carlos A. Fernandes, E. A. Hartmann, R. A. Ortega-Minakata, L. Sampedro, Ramachrisna Teixeira, P. Amram, Daniela Lazzaro, N. Muñoz-Elgueta, R. Lopes de Oliveira, C. H. Veiga, E. Pattaro, Teresa Santos-Silva, C. B. Pereira, S. V. Werner, R. Cid Fernandes, F. R. Herpich, Alexandre S. Oliveira, Simone Daflon, R. S. de Souza, J. S. Alcaniz, Analia Viviana Smith Castelli, Beatriz B. Siffert, D. F. De Paula, C. Bonatto, H. D. Perottoni, Marina Trevisan, Y. Jimenez-Teja, Eduardo S. Pereira, L. Sodré, Timothy C. Beers, M. Borges Fernandes, A. Werle, M. L. Buzzo, C. Mendes de Oliveira, M. Castejon, Vinicius M. Placco, Richard L. Donnerstein, Javier Alonso-García, Roderik Overzier, S. Bonoli, J. A. Hernandez-Jimenez, C. Queiroz, Beatriz Luci Fernandes, Rodolfo H. Barbá, R. Monteiro-Oliveira, Thiago S. Gonçalves, R. Silva, Alvaro Alvarez-Candal, Arianna Cortesi, G. Fabiano de Souza, Karín Menéndez-Delmestre, Eduardo S. Cypriano, T. Ribeiro, J. Caffer, Zach Cano, Martin Makler, S. Fontes, H. S. Xavier, C. L. Barbosa, V. Jatenco-Pereira, K. G. Diem, Amanda R. Lopes, M. L. L. Dantas, R. C. Thom de Souza, A. Galarza, Jane Gregorio-Hetem, J. L. Nilo Castellón, A. Z. Vitorelli, D. Ortíz, R. de Menezes, Denise R. Gonçalves, Reginaldo Bezerra dos Santos, Jordi Miralda-Escudé, J. D. Hernández-Fernández, R. A. Dupke, Alberto Molino, R. Magalhães, L. Riguccini, A. Campillay, Ribamar R. R. Reis, Leandro Kerber, Fabricio Ferrari, G. B. Lima Neto, Pedro H. Bernardinelli, Stavros Akras, V. Branco, Devin D. Whitten, Luis Raul Weber Abramo, P. M. Novais, Antonio D. Montero-Dorta, S. Torres-Flores, Eduardo Telles, J. M. Carvano, C. E. Barbosa, R. de la Reza, Paulo A. A. Lopes, Alessandro Ederoclite
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 489:3403-3411
In this study we define a new sample of distant powerful radio galaxies in order to study their host-galaxy properties and provide targets for future observations of HI absorption with new radio telescopes and to understand the fuelling and feedback
Publikováno v:
Revista UniVap, Vol 19, Iss 34 (2013)
As instabilidades Kelvin-Helmholtz são comuns em sistemas astrofísicos e vão desde jatos deburacos negros até disco de acreção protoplantário. Um objeto astrofísico com fortes características da instabilidade de Kelvin-Helmholtz é a Nebulos
Externí odkaz:
https://doaj.org/article/54b123c5105e418fad266870e5208b18