activity
20012021
most citedWX Cen (= WR 48c) - a possible type Ia Supernova progenitor

19 citations · 53 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2021★ 9 cited

Breaking the degeneracy in magnetic cataclysmic variable X-ray spectral modeling using X-ray light curves

Diogo Belloni, Claudia V. Rodrigues, Matthias R. Schreiber +12

We present an analysis of mock X-ray spectra and light curves of magnetic cataclysmic variables using an upgraded version of the 3D CYCLOPS code. This 3D representation of the accr…

astro-ph.SR2019★ 6 cited

Optical observations and cyclops post-shock region modelling of the polar V348 Pav

Alexandre S. Oliveira, Claudia V. Rodrigues, Matheus S. Palhares +3

Post-shock regions (PSR) of polar cataclysmic variables produce most of their luminosity and give rise to high circular polarization in optical wavelengths and strong variability o…

astro-ph.SR2017

Analysis Of Kepler-71 Activity Through Planetary Transit

Eber A. Gusmão, Caius L. Selhorst, Alexandre S. Oliveira

An exoplanet transiting in front of the disk of its parent star may hide a dark starspot causing a detectable change in the light curve, that allows to infer physical characteristi…

astro-ph.GA2010

The Active Nucleus in NGC 4579

Roberto B. Menezes, João E. Steiner, Tiago V. Ricci +1

In this work, we present an analysis of a data cube obtained with the instrument IFU/GMOS Gemini North telescope centered on the nuclear region of the LINER galaxy NGC 4579. This g…

astro-ph.CO2010

The nature of the LINER in the galaxy NGC 404

Roberto B. Menezes, João E. Steiner, Tiago V. Ricci +1

NGC 404, at a distance of 3.4 Mpc, is the nearest S0 galaxy. This galaxy harbors a LINER; however, since the spectrum does not show a broad Hα emission, it is not certain that this…

astro-ph2005

A hot story with many tales: the qWR star HD 45166. I- Observations and system parameters

J. E. Steiner, Alexandre Oliveira

The binary star HD 45166 has been observed since 1922 but its orbital period has not yet been found. It is considered a peculiar Wolf-Rayet star, and its assigned classification va…