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On the Search for the Galactic PeVatrons by Means of Gamma-Ray Astronomy

open access: yesUniverse, 2022
Cosmic rays are ultra-relativistic particles that slam into the atmosphere from all directions in the sky. Gamma rays emitted when cosmic rays interact with Galactic gas and radiation fields are a powerful tool to investigate their origin. Many candidate
Sabrina Casanova
doaj   +2 more sources

Quiescent and Active Galactic Nuclei as Factories of Merging Compact Objects in the Era of Gravitational Wave Astronomy [PDF]

open access: yesUniverse, 2023
Galactic nuclei harbouring a central supermassive black hole (SMBH), possibly surrounded by a dense nuclear cluster (NC), represent extreme environments that house a complex interplay of many physical processes that uniquely affect stellar formation ...
M. A. Sedda, S. Naoz, B. Kocsis
semanticscholar   +1 more source

Latest results from the DAMPE space mission [PDF]

open access: yesEPJ Web of Conferences, 2023
The space-based DAMPE (DArk Matter Particle Explorer) particle detector has been taking data for more than 7 years since its successful launch in December 2015.
Cagnoli Irene   +2 more
doaj   +1 more source

Exploring the high energy frontiers of the Milky Way with ground-based gamma-ray astronomy: PeVatrons and the quest for the origin of Galactic cosmic-rays [PDF]

open access: yesTurkish Journal of Physics, 2023
Cosmic rays (CRs) are charged particles that arrive at Earth isotropically from all directions and interact with the atmosphere. The presence of a spectral knee feature seen in the CR spectrum at $\sim$3 PeV energies is an evidence that astrophysical ...
E. Angüner
semanticscholar   +1 more source

Galactic ChitChat: Using Large Language Models to Converse with Astronomy Literature [PDF]

open access: yesResearch Notes of the AAS, 2023
We demonstrate the potential of the state-of-the-art OpenAI GPT-4 large language model to engage in meaningful interactions with Astronomy papers using in-context prompting.
I. Ciucă, Y. Ting
semanticscholar   +1 more source

Near-infrared Flux Distribution of Sgr A* from 2005–2022: Evidence for an Enhanced Accretion Episode in 2019

open access: yesThe Astrophysical Journal Letters, 2023
Sgr A* is the variable electromagnetic source associated with accretion onto the Galactic center supermassive black hole. While the near-infrared (NIR) variability of Sgr A* was shown to be consistent over two decades, unprecedented activity in 2019 ...
Grant C. Weldon   +12 more
doaj   +1 more source

Mass distribution in the Galactic Center based on interferometric astrometry of multiple stellar orbits [PDF]

open access: yesAstronomy & Astrophysics, 2021
The stars orbiting the compact radio source Sgr A* in the Galactic Centre are precision probes of the gravitational field around the closest massive black hole.
G. C. R. Abuter   +63 more
semanticscholar   +1 more source

The FAST Galactic Plane Pulsar Snapshot survey: I. Project design and pulsar discoveries [PDF]

open access: yesResearch in Astronomy and Astrophysics, 2021
Discovery of pulsars is one of the main goals for large radio telescopes. The Five-hundred-meter Aperture Spherical radio Telescope (FAST), that incorporates an L-band 19-beam receiver with a system temperature of about 20 K, is the most sensitive radio ...
J. Han   +36 more
semanticscholar   +1 more source

The globular cluster VVV CL002 falling down to the hazardous Galactic centre [PDF]

open access: yesAstronomy & Astrophysics, 2023
The Galactic centre is hazardous for stellar clusters because of the strong tidal force in action there. It is believed that many clusters were destroyed there and contributed stars to the crowded stellar field of the bulge and the nuclear stellar ...
Dante Minniti   +17 more
semanticscholar   +1 more source

Einstein’s Geometrical versus Feynman’s Quantum-Field Approaches to Gravity Physics: Testing by Modern Multimessenger Astronomy

open access: yesUniverse, 2020
Modern multimessenger astronomy delivers unique opportunity for performing crucial observations that allow for testing the physics of the gravitational interaction.
Yurij Baryshev
doaj   +1 more source

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