activity
19972023
most citedEvidence for reduced magnetic braking in polars from binary population models

78 citations · 606 across the 43 of their papers we have counts for

collaborators

44 papers

astro-ph.GA2023★ 15 cited

Interstellar Polarization Survey III: Relation Between Optical Polarization and Reddening in the General Interstellar Medium

Y. Angarita, M. J. F. Versteeg, M. Haverkorn +4

Optical starlight can be partially polarized while propagating through the dusty, magnetized interstellar medium. The polarization efficiency describes the polarization intensity f…

astro-ph.GA2022★ 18 cited

Interstellar Polarization Survey II: General Interstellar Medium

M. J. F. Versteeg, A. M. Magalhães, M. Haverkorn +4

Magnetic fields permeate the entire Galaxy and are essential to, for example, the regulation of several stages of the star formation process and cosmic ray transportation. Unraveli…

astro-ph.HE2022

Evidence for 3XMM J185246.6+003317 as a massive magnetar with a low magnetic field

Rafael C. R. de Lima, Jonas P. Pereira, Jaziel G. Coelho +10

3XMM J185246.6+003317 is a transient magnetar located in the vicinity of the supernova remnant Kes\,79. So far, observations have only set upper limits to its surface magnetic fiel…

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.SR2021★ 7 cited

Search for magnetic accretion in SW Sextantis systems

I. J. Lima, C. V. Rodrigues, C. E. Ferreira Lopes +9

SW Sextantis systems are nova-like cataclysmic variables that have unusual spectroscopic properties, which are thought to be caused by an accretion geometry having part of the mass…

astro-ph.HE2020★ 16 cited

A magnetic white-dwarf accretion model for the anomalous X-ray pulsar 4U 0142+61

Sarah V. Borges, Claudia V. Rodrigues, Jaziel G. Coelho +2

The quiescent emission of the anomalous X-ray pulsar (AXP) 4U 0142+61 extends over a broad range of energy, from radio up to hard X-rays. In particular, this object is unique among…