activity
20022008
most citedMassive stars exploding in a He-rich circumstellar medium. I. Type Ibn (SN 2006jc-like) events

203 citations · 653 across the 11 of their papers we have counts for

collaborators

7 papers

astro-ph200825 cited

Outliers from the mainstream: how a massive star can produce a gamma-ray burst

S. Campana, N. Panagia, D. Lazzati +12

It is now recognized that long-duration Gamma-Ray Bursts (GRBs) are linked to the collapse of massive stars, based on the association between (low-redshift) GRBs and (type Ic) core…

astro-ph200858 cited

The complex light-curve of the afterglow of GRB071010A

S. Covino, P. D'Avanzo, A. Klotz +51

We present and discuss the results of an extensive observational campaign devoted to GRB071010A, a long-duration gamma-ray burst detected by the Swift satellite. This event was fol…

astro-ph20082 cited

Novae as a Class of Transient X-ray Sources

K. Mukai, M. Orio, M. Della Valle

Motivated by the recently discovered class of faint (10^34-10^35 ergs/s) X-ray transients in the Galactic Center region, we investigate the 2-10 keV properties of classical and rec…

astro-ph2008203 cited

Massive stars exploding in a He-rich circumstellar medium. I. Type Ibn (SN 2006jc-like) events

A. Pastorello, S. Mattila, L. Zampieri +26

We present new spectroscopic and photometric data of the type Ibn supernovae 2006jc, 2000er and 2002ao. We discuss the general properties of this recently proposed supernova family…

astro-ph200636 cited

Early spectral evolution of Nova Sgr 2004 (V5114 Sgr)

A. Ederoclite, E. Mason, M. Della Valle +15

We present optical and near-infrared spectral evolution of the Galactic nova V5114 Sgr (2004) during few months after the outburst. We use multi-band photometry and line intensitie…

astro-ph2006104 cited

On the consistency of the peculiar GRBs 060218 and 060614 with the Ep,i - Eiso correlation

L. Amati, M. Della Valle, F. Frontera +4

We analyze and discuss the position of GRB 060218 and GRB 060614 in the Ep,i - Eiso plane. GRB 060218 is important because of its similarity with GRB 980425, the proto-type event o…