activity
20042007
most citedAccretion and ejection properties of embedded protostars: the case of HH26, HH34 and HH46 IRS

87 citations · 130 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph200713 cited

Tracing the origins of permitted emission lines in RU Lupi down to AU scales

L. Podio, P. J. V. Garcia, F. Bacciotti +4

Most of the observed emission lines and continuum excess from young accreting low mass stars (Classical T Tauri stars -- CTTSs) take place in the star-disk or inner disk region. Th…

astro-ph200787 cited

Accretion and ejection properties of embedded protostars: the case of HH26, HH34 and HH46 IRS

S. Antoniucci, B. Nisini, T. Giannini +1

We present the results of a near-IR spectroscopic analysis on 3 young embedded sources (HH26IRS, HH34IRS and HH46IRS) belonging to different star-forming regions and displaying wel…

astro-ph200630 cited

Evidence for T Tauri-like emission in the EXor V1118 Ori from near-IR and X-ray data

D. Lorenzetti, T. Giannini, L. Calzoletti +6

We present a near-IR study of the EXor variable V1118 Ori, performed by following a slightly declining phase after a recent outburst. In particular, the near-IR (0.8 - 2.3 micron)…

astro-ph2004

VINCI-VLTI measurements of HR 4049: the physical size of the circumbinary envelope

Simone Antoniucci, Francesco Paresce, Markus Wittkowski

We present the first detection of the envelope which surrounds the post-AGB binary source HR 4049. VINCI-VLTI K-band interferometric observations of this source imply the existence…

astro-ph2004

Probing the embedded YSOs of the R CrA region through VLT-ISAAC spectroscopy

B. Nisini, S. Antoniucci, T. Giannini +1

Near IR spectra obtained with ISAAC at VLT, have been used to pose constraints on the evolutionary state and accretion properties of a sample of five embedded YSOs located in the R…

astro-ph2004

Observations of the Brackett decrement in the Class I source HH100 IR

Brunella Nisini, Simone Antoniucci, Teresa Giannini

The Brackett decrement in the Class I source HH100 IR has been observed and analyzed to set constraints on the origin of the IR HI emission in this young object. We have used both…