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
Showing astro-ph.SRShow all

6 papers · 1 filter

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.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-…

astro-ph.SR2021

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…

astro-ph.SR2018★ 9 cited

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…

astro-ph.SR2016★ 14 cited

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…

astro-ph.SR2015★ 7 cited

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…