Results 61 to 70 of about 207,256 (183)
Gamma ray emission from embedded young massive star clusters unveiled by Fermi-LAT [PDF]
Massive star clusters (SCs) have been proposed as additional contributors to Galactic Cosmic rays (CRs), to overcome the limitations of supernova remnants (SNR) to reach the highest energy end of the Galactic CR spectrum.
Peron Giada +3 more
doaj +1 more source
Galactic Superaccreting X-Ray Binaries as Super-PeVatron Accelerators
The extension of the cosmic-ray (CR) spectrum well beyond 1 PeV necessitates the existence of a population of accelerators in the Milky Way, which we refer to as super-PeVatrons. Identifying the nature of these sources remains a challenge to the paradigm
Jieshuang Wang +2 more
doaj +1 more source
The Spatially Resolved Hot Gas Properties of NGC 1266’s Active Galactic Nucleus-driven Outflow
Galactic winds play a critical role in galaxy evolution, yet their structure and driving mechanisms remain poorly understood, especially in low-luminosity active galactic nucleus (LLAGN) systems.
Sebastian Lopez +4 more
doaj +1 more source
Feedback from active galactic nuclei (AGN) is widely acknowledged to regulate the growth of massive galaxies, though its driving mechanisms are debated.
Elise Fuller +18 more
doaj +1 more source
Wind-fed Supermassive Black Hole Accretion in the Ultracompact Dwarf Galaxy M60-UCD1
Ultracompact dwarf galaxies (UCDs) are thought to be remnants of stripped galactic nuclei, among which a handful are known to host a central supermassive black hole (SMBH).
Zhao Su, Zhiyuan Li, Meicun Hou
doaj +1 more source
We report the small-scale spatial variation in cool ( T ∼ 10 ^4 K) Mg ii absorption detected in the circumgalactic medium (CGM) of a star-forming galaxy at z ≈ 0.8.
Ahmed Shaban +8 more
doaj +1 more source
A Dual Active Black Hole Candidate with Mass Ratio ~7:1 in a Disk Galaxy
Dual active galactic nuclei (AGNs) with comparable masses are commonly witnessed among the major merged galaxies with interaction remnants. Considering almost every massive galaxy is associated with multiple dwarf satellites around it, minor mergers ...
Xiao Cao +10 more
doaj +1 more source
Feedback-driven massive outflows play a crucial role in galaxy evolution by regulating star formation and influencing the dynamics of surrounding media. Extracting outflow properties from spectral lines is a notoriously difficult process for a number of ...
Mason Huberty +19 more
doaj +1 more source
Elemental abundances in AGB stars and the formation of the Galactic bulge
We obtained high-resolution near-IR spectra of 45 AGB stars located in the Galactic bulge. The aim of the project is to determine key elemental abundances in these stars to help constrain the formation history of the bulge.
Wood P.R. +6 more
doaj +1 more source
12 pages, 7 figures, accepted for publication in the Astrophysical ...
Dawson, Steve +6 more
openaire +2 more sources

