Results 31 to 40 of about 5,123,669 (303)
TROJAN STARS IN THE GALACTIC CENTER [PDF]
17 pages, 9 figures, accepted for publication in ...
Fujii, Michiko +3 more
openaire +2 more sources
Sources and Radiations of the Fermi Bubbles
Two enigmatic gamma-ray features in the galactic central region, known as Fermi Bubbles (FBs), were found from Fermi-LAT data. An energy release, (e.g., by tidal disruption events in the Galactic Center, GC), generates a cavity with a shock that expands ...
Vladimir A. Dogiel, Chung-Ming Ko
doaj +1 more source
Jet from the Milky Way center: the galactic center lobe
The radio lobe in the galactic center found through 10-GHz continuum observations is likely to be a cylindrical jet emerging from the nuclear disk of the Milky Way Galaxy.
Yoshiaki Sofue
core +1 more source
The distance to the galactic center [PDF]
Methods used to determine the distance (R₀) to the galactic center are described and recent results are presented. These suggest that R₀≃7 Kpc.
Blanco, V.M.
core
Despite a decade’s worth of gravitational wave observations, the origin of the binary black hole (BBH) mergers detected by the LIGO–Virgo–KAGRA (LVK) collaboration remains an open question.
Yubo Su
doaj +1 more source
After more than a decade since its discovery, the Galactic center gamma-ray excess - discovered with the Fermi Large Area Telescope - remains puzzling. While the spectrum of the signal can be explained by either dark matter or an unresolved population of
Oscar Macias, Martin Pohl, Chris Gordon, Phaedra Coleman
doaj +1 more source
The Galactic Center in Color: Measuring Extinction with High-proper-motion Stars
The Milky Way’s central parsec is a highly extinguished region with a population of high-proper-motion stars. We have tracked 145 stars for ∼10 yr at wavelengths between 1 and 4 μ m to analyze extinction effects in color–magnitude space. Approximately 30%
Zoë Haggard +8 more
doaj +1 more source
Star Formation in the Galactic Center
Research on Galactic Center star formation is making great advances, in particular due to new data from interferometers spatially resolving molecular clouds in this environment.
Jens Kauffmann
core +1 more source
ABSTRACT Objective Neurochemical levels measured by brain MR spectroscopy (MRS) have been proposed as endpoints for clinical trials in early‐stage spinocerebellar ataxia (SCA) trials. We tested their trial‐readiness by quantifying neurochemicals in three affected brain regions in early‐stage cohorts of SCA2 and SCA3, examining their reproducibility in ...
James M. Joers +19 more
wiley +1 more source
Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar Collisions
The dense concentration of stars and high-velocity dispersions in the Galactic center imply that stellar collisions frequently occur. Stellar collisions could therefore result in significant mass loss rates.
Douglas Rubin, Abraham Loeb
doaj +1 more source

