Searh results
RESEARCH ACTIVITIES IN HIGH-ENERGY ASTROPHYSICS
Volume 93, n. 2-3, 2022
O. Straniero | Stars and physics beyond the Standard Model DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.1 |
E. Orlando | The high-energy emission from the quiet Sun DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.2 |
T. Belloni et al. | DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.3 |
G. Israel et al. | DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.4 |
M. Orio | X-ray observations of accreting and burning white dwarfs DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.5 |
M. Brusa et al. | Supermassive Black Hole Winds in X–rays DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.6 |
M. Dadina et al. | Probing AGN feedback in the most luminous QSO at cosmic noon DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.7 |
G. Risaliti et al. | Quasars at High-Redshift: Physics and Cosmology DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.8 |
P. Severgnini et al. | Supermassive Black Hole Binaries and dual AGN DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.9 |
E. Torresi et al. | Exploring the radio morphology-accretion mode link in radio galaxies at high energies DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.10 |
E. Pian et al. | Probing the physics of compact extragalactic sources over multiple scales DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.11 |
S. Andreon & F. Castagna | Our approach to the thermodynamic evolution of galaxy clusters DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.12 |
S. Ettori et al. | Galaxy clusters in X-rays: the buildup of massive structures in the last 10 Gyrs, and CHEX-MATE DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.13 |
A. Moretti et al. | DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.14 |
P. Tozzi et al. | Mapping Feedback Processes in the Intracluster Medium at low and high redshift DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.15 |
A. De Luca et al. | The ULTraS project: Understanding the X-ray variable and transient sky DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.16 |
G. Stratta et al. | On the origin of afterglow ”plateaus” in gamma-ray bursts DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.17 |
G. Ghisellini et al. | The new age of Gamma Ray Bursts: physics and multi-messengers DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.18 |
C. Guidorzi et al. | A search for high-energy counterparts to extragalactic fast radio burst sources with Insight–HXMT DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.19 |
M. Bertaina et al | DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.20 |
E. Amato et al. | On the escape of cosmic ray leptons and their impact on the background plasma DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.21 |
P. Blasi et al. | A Modern Approach to Cosmic Ray Transport in the Galaxy DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.22 |
F. Donato & S. Recchia | nverse Compton halos around Pulsar Wind Nebulae DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.23 |
S. Orlando et al. | Connecting supernova remnants to their parent supernovae DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.24 |
M. Regis et al. | Deciphering the high-energy sky via angular cross correlations DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.25 |
E. Caroli et al. | 3DCaTM: a 3D Cadmium Zinc Telluride spectroscopic module for hard X- and γ-ray astronomy DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.26 |
O. Catalano et al. | FluChe: Fluorescence and Cherenkov light detection with SiPM for space and ground applications DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.27 |
E. Virgilli et al. | DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.28 |
R. Gilli et al. | Next Generation X-ray Imaging Surveys DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.29 |
A. De Rosa et al. | DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.30 |
D. D’Urso, et al. | POX – PANGU Optimization and eXperimental verification: design and perfor- mance DOI: https://doi.org/10.36116/MEMSAIT_93N2_3.2022.31 |
