Zobrazeno 1 - 10
of 1 453
pro vyhledávání: '"Fernandes, I"'
Autor:
Fernandes, I. L., Cabrera, G. G.
Based on Keldysh non-equilibrium Green function method, we have investigated spin current production in a hybrid T-shaped device, consisting of a central quantum dot connected to the leads and a side dot which only couples to the central dot. The top
Externí odkaz:
http://arxiv.org/abs/1802.03439
Autor:
Fonseca, P. G., Neves, E. P. S., Soares, M. E. C., Galo, R., Ramos-Jorge, M. L., Fernandes, I. B.
Publikováno v:
European Archives of Paediatric Dentistry (Springer Science & Business Media B.V.); Oct2024, Vol. 25 Issue 5, p715-720, 6p
Autor:
Faundez-Abans, M., de Oliveira-Abans, M., Krabbe, A. C., da Rocha-Poppe, P. C., Fernandes-Martin, V. A., Fernandes, I. F.
Publikováno v:
A&A 558, A13 (2013)
Aims. We investigate the nature of the galaxy pair FM 047-02, which has been proposed as an archetype of the Solitaire types of peculiar (collisional) ring galaxies. Methods. The study is based on long-slit spectrophotometric data in the range of 350
Externí odkaz:
http://arxiv.org/abs/1310.6807
Interactions between galaxies are very common. There are special kinds of interactions that produce systems called Polar Ring Galaxies (PRGs), composed by a lenticular, elliptical, or spiral host galaxy, surrounded by a ring of stars and gas, orbitin
Externí odkaz:
http://arxiv.org/abs/1208.3421
Autor:
Faúndez-Abans, M., Krabbe, A. C., Oliveira-Abans, M., Poppe, P. C. da Rocha, Rodrigues, I., Martin, V. A. Fernandes, Fernandes, I. F.
We report first results of an investigation of the tidally disturbed galaxy system AM\,546-324, whose two principal galaxies 2MFGC 04711 and AM\,0546-324 (NED02) were previously classified as interacting doubles. This system was selected to study the
Externí odkaz:
http://arxiv.org/abs/1206.0719
Autor:
Silva, T. M., Nascimento, C. F. G., Teixeira, I. A. R., Lima, K. P. B. A., Fernandes, I. V., Oliveira, M. C. B. M., Monteiro, E. C. B., Melo Neto, A. A., Delgado, J. M. P. Q.
Publikováno v:
Journal of Building Pathology & Rehabilitation; 5/11/2024, Vol. 9 Issue 2, p1-19, 19p
Publikováno v:
Mon.Not.Roy.Astron.Soc.364:674-682,2005
When analysing HII regions, a possible source of systematic error on empirically derived physical quantities is the limited size of the slit used for the observations. A grid of photoionization models was built through the Aangaba code varying the io
Externí odkaz:
http://arxiv.org/abs/astro-ph/0509345
We analyze longslit spectral observations of fourteen Wolf-Rayet galaxies from the sample of Schaerer, Contini & Pindao (1999). All 14 galaxies show broad Wolf-Rayet emission in the blue region of the spectrum, consisting of a blend of NIII4640, CIII
Externí odkaz:
http://arxiv.org/abs/astro-ph/0409114
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Akademický článek
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