229 citations · 1.8k across the 51 of their papers we have counts for
52 papers
Morphological properties of the Crab Nebula: a detailed multiwavelength study based on new VLA, HST, Chandra and XMM-Newton images
G. Dubner, G. Castelletti, O. Kargaltsev +3
We present a detailed analysis of the morphological properties of the Crab Nebula across the electromagnetic spectrum based on new and previous high-quality data from radio to X-ra…
Modeling the shock-cloud interaction in SN 1006: unveiling the origin of nonthermal X-ray and gamma-ray emission
Marco Miceli, Salvatore Orlando, Victor Pereira +9
The supernova remnant SN 1006 is a source of high-energy particles and its southwestern limb is interacting with a dense ambient cloud, thus being a promising region for gamma-ray…
Feature-tailored spectroscopic analysis of the SNR Puppis A in X-rays
G. J. M. Luna, M. J. S. Smith, G. Dubner +2
We introduce a distinct method to perform spatially-resolved spectral analysis of astronomical sources with highly structured X-ray emission. The method measures the surface bright…
HESS J1943+213: a non-classical high-frequency-peaked BL Lac object
Samayra M. Straal, Krisztina E. Gabanyi, Joeri van Leeuwen +5
HESS J1943+213 is an unidentified TeV source that is likely a high-frequency-peaked BL Lac (HBL) object but also compatible with a pulsar wind nebula (PWN) nature. Each of these en…
Interactions of the Infrared bubble N4 with the surroundings
Hong-Li Liu, Jin-Zeng Li, Yuefang Wu +11
The physical mechanisms that induce the transformation of a certain mass of gas in new stars are far from being well understood. Infrared bubbles associated with HII regions have b…
Deep morphological and spectral study of the SNR RCW 86 with Fermi-LAT
LAT Collaboration, G. Dubner, L. Duvidovich +4
RCW 86 is a young supernova remnant (SNR) showing a shell-type structure at several wavelengths and is thought to be an efficient cosmic-ray (CR) accelerator. Earlier \textit{Fermi…