activity
20152026
most citedNegative and Positive Feedback from a Supernova Remnant with SHREC: A detailed Study of the Shocked Gas in IC443

27 citations · 133 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2026

Probing the potential high-energy messengers of the anticipated T Coronae Borealis outburst

O. Petruk, T. Kuzyo, S. Orlando +4

T Coronae Borealis (T CrB) is a nearby recurrent nova expected to erupt in the near future, offering a unique opportunity to study particle acceleration and high-energy emission fr…

astro-ph.HE2025★ 8 cited

Tracing the ejecta structure of SN 1987A: Insights and diagnostics from 3D MHD simulations

S. Orlando, M. Miceli, M. Ono +14

Supernova (SN) 1987A provides a unique window into the aftermath of a massive stellar explosion, offering key insights into the ejecta's morphology, composition, explosion mechanis…

astro-ph.GA2023★ 4 cited

Rubin LSST observing strategies to maximize volume and uniformity coverage of Star Forming Regions in the Galactic Plane

L. Prisinzano, R. Bonito, A. Mazzi +9

A complete map of the youngest stellar populations of the Milky Way in the era of all-sky surveys, is one of the most challenging goals in modern astrophysics. The characterisation…

astro-ph.SR2023★ 13 cited

Young stellar objects, accretion disks, and their variability with Rubin Observatory LSST

R. Bonito, L. Venuti, S. Ustamujic +14

Vera C. Rubin Observatory, through the Legacy Survey of Space and Time (LSST), will allow us to derive a panchromatic view of variability in young stellar objects (YSOs) across all…

astro-ph.IM2022★ 3 cited

From Data to Software to Science with the Rubin Observatory LSST

Katelyn Breivik, Andrew J. Connolly, K. E. Saavik Ford +97

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) dataset will dramatically alter our understanding of the Universe, from the origins of the Solar System to the…

astro-ph.SR2022★ 4 cited

Pre main sequence: Accretion & Outflows

P. Christian Schneider, H. Moritz Günther, Sabina Ustamujic

Low-mass pre-main sequence (PMS) stars are strong X-ray sources, because they possess hot corona like their older main-sequence counterparts. Unique to young stars, however, are X-…