activity
20162022
most citedConstraints on the structure and seasonal variations of Triton's atmosphere from the 5 October 2017 stellar occultation and previous observations

20 citations · 80 across the 9 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2022★ 20 cited

Constraints on the structure and seasonal variations of Triton's atmosphere from the 5 October 2017 stellar occultation and previous observations

J. Marques Oliveira, B. Sicardy, A. R. Gomes-Júnior +234

A stellar occultation by Neptune's main satellite, Triton, was observed on 5 October 2017 from Europe, North Africa, and the USA. We derived 90 light curves from this event, 42 of…

astro-ph.SR2020★ 4 cited

Long-term photospheric instabilities and envelopes dynamics in the post-AGB binary system 89 Herculis

M. Gangi, M. Giarrusso, M. Munari +3

We present a long-term optical spectroscopic study of the post-AGB binary system 89 Herculis, with the aim to characterize the relationship between photospheric instabilities and d…

astro-ph.SR2018★ 3 cited

The solar-like "Second Spectrum" and the polarised metal lines in emission of the post-AGB binary 89 Herculis

F. Leone, M. Gangi, M. Giarrusso +6

We studied the polarised spectrum of the post-AGB binary system 89\,Herculis on the basis of data collected with the high resolution \emph{Catania Astrophysical Observatory Spectro…

astro-ph.SR2017★ 12 cited

The multi-line slope method for the measure of the effective magnetic field of the cool stars: an application to the solar like cycle of ε Eri

C. Scalia, F. Leone, M. Gangi +2

A method for the determination of integrated longitudinal stellar fields from low-resolution spectra is the so-called slope method, which is based on the regression of the Stokes V…

astro-ph.SR2017★ 14 cited

A method to measure the transverse magnetic field and orient the rotational axis of stars

Francesco Leone, Cesare Scalia, Manuele Gangi +5

Direct measurements of the stellar magnetic fields are based on the splitting of spectral lines into polarized Zeeman components. With few exceptions, Zeeman signatures are hidden…

astro-ph.SR2017★ 1 cited

Estimating the chromospheric magnetic field from a revised NLTE modeling: the case of HR7428

Innocenza Busa, Giovanni Catanzaro, Antonio Frasca +6

In this work we use the semi-empirical atmospheric modeling method to obtain the chro-mospheric temperature, pressure, density and magnetic field distribution versus height in the…

astro-ph.SR2016★ 10 cited

A spectroscopic study of the open cluster NGC 6250

A. J. Martin, M. J. Stift, L. Fossati +4

We present the chemical abundance analysis of 19 upper main-sequence stars of the young open cluster NGC 6250 (log t ~ 7.42 yr). This work is part of a project aimed at setting obs…