27 citations · 133 across the 14 of their papers we have counts for
14 papers
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…
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…
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…
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…
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…
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-…
Negative and Positive Feedback from a Supernova Remnant with SHREC: A detailed Study of the Shocked Gas in IC443
G. Cosentino, I. Jiménez-Serra, J. C. Tan +20
Supernova remnants (SNRs) contribute to regulate the star formation efficiency and evolution of galaxies. As they expand into the interstellar medium (ISM), they transfer vast amou…
Modeling the Remnants of Core-collapse Supernovae from Luminous Blue Variable stars
S. Ustamujic, S. Orlando, M. Miceli +8
LBVs are massive evolved stars that suffer sporadic and violent mass-loss events. They have been proposed as the progenitors of some core-collapse SNe, but this idea is still debat…
Modeling particle acceleration and non-thermal emission in supernova remnants
S. Orlando, M. Miceli, S. Ustamujic +5
According to the most popular model for the origin of cosmic rays (CRs), supernova remnants (SNRs) are the site where CRs are accelerated. Observations across the electromagnetic s…
Modeling the mixed-morphology supernova remnant IC 443. Origin of its complex morphology and X-ray emission
S. Ustamujic, S. Orlando, E. Greco +4
The morphology and the distribution of material observed in SNRs reflect the interaction of the SN blast wave with the ambient environment, the physical processes associated with t…
3D modeling from the onset of the SN to the full-fledged SNR: Role of an initial ejecta anisotropy on matter mixing
Antonio Tutone, Salvatore Orlando, Marco Miceli +8
The aim of this work is to bridge the gap between CC SNe and their remnants by investigating how post-explosion anisotropies in the ejecta influence the structure and chemical prop…
Structure of X-ray emitting jets close to the launching site: from embedded to disk-bearing sources
S. Ustamujic, S. Orlando, R. Bonito +2
Several observations of stellar jets show evidence of X-ray emitting shocks close to the launching site. In some cases, the shocked features appear to be stationary, also for YSOs…
Formation of X-ray emitting stationary shocks in magnetized protostellar jets
S. Ustamujic, S. Orlando, R. Bonito +3
X-ray observations of protostellar jets show evidence of strong shocks heating the plasma up to temperatures of a few million degrees. In some cases, the shocked features appear to…
X-ray emission from stellar jets by collision against high-density molecular clouds: an application to HH 248
Javier Lopez-Santiago, Rosaria Bonito, Mariana Orellana +6
We investigate the plausibility of detecting X-ray emission from a stellar jet that impacts against a dense molecular cloud. This scenario may be usual for classical T Tauri stars…