activity
20022026
most citedWind-Wind Collision in the eta Carinae Binary System: a Shell-Like Event Near Periastron

41 citations · 309 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.SR2026

Magnetically Confined Mountains on Accreting White Dwarfs

Pedro H. B. Rossetto, Manoel F. Sousa, Diego A. Falceta-Gonçalves

The hydromagnetic structure of magnetically confined mountains on accreting white dwarfs is computed, alongside the effects of accretion on the reduction of the star's magnetic fie…

astro-ph.SR2022★ 1 cited

Telluric absorption lines in the ALMA spectra of Car

Zulema Abraham, Pedro. P. B. Beaklini, Pierre Cox +2

The massive binary system formed by Car and an unknown companion is a strong source at millimetre and submillimetre wavelengths. Close to the stars, continuum bremsstrahlung an…

astro-ph.SR2020★ 6 cited

Carinae: high angular resolution continuum, H30 and He30 ALMA images

Z. Abraham, P. P. B. Beaklini, P. Cox +2

We present images of Carinae in the recombination lines H30 and He30 and the underlying continuum with 50~mas resolution (110 AU), obtained with ALMA. For the first time,…

astro-ph.HE2015★ 2 cited

Magnetic fields, non-thermal radiation and particle acceleration in colliding winds of WR-O stars

D. Falceta-Goncalves

Non-thermal emission has been detected in WR-stars for many years at long wavelengths spectral range, in general attributed to synchrotron emission. Two key ingredients are needed…

astro-ph.SR2014★ 24 cited

Carinae Baby Homunculus Uncovered by ALMA

Zulema Abraham, Diego Falceta-Gonçalves, Pedro P. B. Beaklini

We report observations of Carinae obtained with ALMA in the continuum of 100, 230, 280 and 660 GHz in 2012 November, with a resolution that varied from 2.88" to 0.45" for the l…

astro-ph.CO2012★ 19 cited

The mass loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts

Luciana O. Ruiz, Diego Falceta-Gonçalves, Gustavo A. Lanfranchi +1

Theoretical CDM cosmological models predict a much larger number of low mass dark matter haloes than has been observed in the Local Group of galaxies. One possible explanation i…