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19992026
most citedFilaments and ridges in Vela C revealed by Herschel: from low-mass to high-mass star-forming sites

240 citations · 4.2k across the 126 of their papers we have counts for

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Showing 2017 · astro-ph.SRShow all

5 papers · 2 filters

astro-ph.SR2017★ 11 cited

The 2016-2017 peak luminosity of the pre-main sequence variable V2492 Cyg

T. Giannini, U. Munari, S. Antoniucci +5

V2492 Cyg is a young pre-main sequence star presenting repetitive brightness variations of significant amplitude (Delta R > 5 mag) whose physical origin has been ascribed to both e…

astro-ph.SR2017★ 106 cited

Connection between jets, winds and accretion in T Tauri stars: the X-shooter view

B. Nisini, S. Antoniucci, J. M. Alcala' +5

We have analysed the [OI]6300 A line in a sample of 131 young stars with discs in the Lupus, Chamaeleon and signa Orionis star forming regions, observed with the X-shooter spectrog…

astro-ph.SR2017★ 14 cited

High-resolution TNG spectra of T Tauri stars: Near-IR GIANO observations of the young variables XZ Tau and DR Tau

S. Antoniucci, B. Nisini, K. Biazzo +6

We used the TNG/GIANO instrument to obtain near-IR high-resolution spectra (R~50000) of XZ Tau and DR Tau, two actively accreting T Tauri stars classified as EXors. The analysis of…

astro-ph.SR2017★ 26 cited

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…

astro-ph.SR2017★ 6 cited

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…