activity
20122023
most citedMultiwavelength flaring activity of PKS1510-089

11 citations · 33 across the 8 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2023

A two-component clumpy model for the shell evolution of classical novae: the case of V5668 Sgr

Zulema Abraham, Larissa Takeda, Pedro P. B. Beaklini +4

The shell of the classical nova V5668 Sgr was resolved by ALMA at the frequency of 230 GHz 927 days after eruption, showing that most of the continuum bremsstrahlung emission origi…

astro-ph.SR20221 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.SR20206 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.GA20203 cited

AGN dichotomy beyond radio loudness: a Gaussian Mixture Model analysis

Pedro P. B. Beaklini, Allan V. C. Quadros, Marcio G. B. de Avellar +2

Since the discovery of Quasi-stellar Objects (QSOs), also known as quasars, they have been traditionally subdivided as radio-loud and radio-quiet sources. Whether such division is…

astro-ph.SR20197 cited

Sulphur-Bearing and Complex Organic Molecules in an Infrared Cold Core

Pedro P. B. Beaklini, Edgar Mendoza, Carla M. Canelo +9

Since the start of ALMA observatory operation, new and important chemistry of infrared cold core was revealed. Molecular transitions at millimeter range are being used to identify…

astro-ph.HE20194 cited

Multiwavelength analysis of brightness variations of 3C~279: Probing the relativistic jet structure and its evolution

Pedro P. B. Beaklini, Tânia P. Dominici, Zulema Abraham +1

We studied the correlation between brightness and polarization variations in 3C~279 at different wavelengths, over time intervals long enough to cover the time lags due to opacity…