285 citations · 1.1k across the 54 of their papers we have counts for
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The 2015-2016 outburst of the classical EXor V1118 Ori
T. Giannini, S. Antoniucci, D. Lorenzetti +15
After a quiescence period of about 10 years, the classical EXor source V1118 Ori has undergone an accretion outburst in 2015 September. The maximum brightness (DV > 4 mag) was reac…
Investigating the past history of EXors: the cases of V1118 Ori, V1143 Ori, and NY Ori
R. Jurdana-Šepić, U. Munari, S. Antoniucci +3
EXor objects are young variables that show episodic variations of brightness commonly associated to enhanced accretion outbursts. With the aim of investigating the long-term photom…
A new insight into the V1184 Tau variability
T. Giannini, D. Lorenzetti, A. Harutyunyan +5
V1184 Tau is a young variable for long time monitored at optical wavelengths. Its variability has been ascribed to a sudden and repetitive increase of the circumstellar extinction…
A long-lasting quiescence phase of the eruptive variable V1118 Ori
D. Lorenzetti, S. Antoniucci, T. Giannini +9
V1118 Ori is an eruptive variable belonging to the EXor class of Pre-Main Sequence stars whose episodic outbursts are attributed to disk accretion events. Since 2006, V1118 Ori is…
Interferometry of chemically peculiar stars: theoretical predictions vs. modern observing facilities
D. Shulyak, C. Paladini, G. Li Causi +2
By means of numerical experiments we explore the application of interferometry to the detection and characterization of abundance spots in chemically peculiar (CP) stars using the…
Mid- and Far-Infrared Variability of PV Cep
Dario Lorenzetti, Simone Antoniucci, Teresa Giannini +4
We present the collection of all the mid- and far-IR observations (3-170 um) of the young eruptive variable PV Cep available so far in the literature. These data allow us to confir…