Showing 41 - 60 results of 66 for search '"Galactic Center', query time: 0.05s Refine Results
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    Hunting for Cold Exoplanets via Microlensing by Beaulieu, Jean-Philippe

    Published 2023-08-01
    “…Microlensing can detect planets at distances ranging from a few hundred parsecs all the way to the Galactic center. The maximum sensitivity is reached for systems that are located half way to the galactic center, with planets orbiting the lens star at a separation of few AUs. …”
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    Evidence for AGN Feedback in Galaxy Clusters and Groups by Myriam Gitti, Fabrizio Brighenti, Brian R. McNamara

    Published 2012-01-01
    “…Instead of the initial idea that the thermal gas is cooling and flowing toward the center, the new picture envisages a complex dynamical evolution of the intracluster medium (ICM) regulated by the radiative cooling and the nongravitational heating from the active galactic nucleus (AGN). …”
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    Observations of Radio Magnetars with the Deep Space Network by Aaron B. Pearlman, Walid A. Majid, Thomas A. Prince

    Published 2019-01-01
    “…When the DSN antennas are not communicating with spacecraft, they provide a valuable resource for performing observations of radio magnetars, searches for new pulsars at the Galactic Center, and additional pulsar-related studies. …”
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    Review of the Empirical Evidence for Superluminal Particles and the 3 + 3 Model of the Neutrino Masses by Robert Ehrlich

    Published 2019-01-01
    “…Furthermore, this dark matter model is supported by several datasets: γ-rays from the galactic center, and the Kamiokande-II neutrino data on the day of SN 1987A. …”
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    Semianalytical Fokker–Planck Models for Nuclear Star Clusters by Karamveer Kaur, Barak Rom, Re’em Sari

    Published 2025-01-01
    “…This improves the rate estimates for extreme-mass ratio inspirals, and has interesting implications for a new class of galactic center transients called quasiperiodic eruptions.…”
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    Recoiling Black Holes: Electromagnetic Signatures, Candidates, and Astrophysical Implications by S. Komossa

    Published 2012-01-01
    “…Supermassive black holes (SMBHs) may not always reside right at the centers of their host galaxies. This is a prediction of numerical relativity simulations, which imply that the newly formed single SMBH, after binary coalescence in a galaxy merger, can receive kick velocities up to several 1000 km/s due to anisotropic emission of gravitational waves. …”
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    A Study of the Star Clusters’ Population in the Giant Molecular Cloud G174+2.5 by Tatyana A. Permyakova, Giovanni Carraro, Anton F. Seleznev, Andrej M. Sobolev, Dmitry A. Ladeyschikov, Maria S. Kirsanova

    Published 2025-01-01
    “…Then, for the detected clusters, we determine their general parameters: the center positions, radii, number of stars, and reddening. …”
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