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Exploring the Evolution of a Dwarf Spheroidal Galaxy with SPH Simulations. II. AGN Feedback
Published 2025-01-01“…We investigate active galactic nucleus (AGN) feedback from an intermediate-mass black hole at the center of a dwarf spheroidal galaxy, by performing isolated galaxy simulations using a modified version of the GADGET-3 code. …”
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The MBH–M∗ Relation up to z ∼ 2 through Decomposition of COSMOS-Web NIRCam Images
Published 2025-01-01Get full text
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Multimessenger Probes of Supermassive Black Hole Spin Evolution
Published 2025-01-01Get full text
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Rare Occasions: Tidal Disruption Events Rarely Power the AGNs Observed in Dwarf Galaxies
Published 2025-01-01Get full text
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Radiation Exposure and Shielding Effects on the Lunar Surface
Published 2024-12-01Get full text
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Dual Jet Interaction, Magnetically Arrested Flows, and Flares in Accreting Binary Black Holes
Published 2025-01-01“…Supermassive binary black holes in galactic centers are potential multimessenger sources in gravitational waves and electromagnetic radiation. …”
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Study of Long-term Spectral Evolution and X-Ray and γ-Ray Correlation of Blazars Seen by HAWC
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Hubble Space Telescope Observations within the Sphere of Influence of the Powerful Supermassive Black Hole in PKS 0745-191
Published 2025-01-01“…We present Space Telescope Imaging Spectrograph observations from the Hubble Space Telescope of the supermassive black hole (SMBH) at the center of PKS 0745-191, a brightest cluster galaxy (BCG) undergoing powerful radio-mode active galactic nucleus (AGN) feedback ( P _cav ~ 5 × 10 ^45 erg s ^−1 ). …”
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Bulk Motions in the Black Hole Jet Sheath as a Candidate for the Comptonizing Corona
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Probing non-standard neutrino interactions with supernova neutrinos at Hyper-K
Published 2020-01-01Get full text
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Hunting for Cold Exoplanets via Microlensing
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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On the Limitations of the Anomalous Microwave Emission Emissivity
Published 2012-01-01Get full text
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Time-resolved Hubble Space Telescope UV Observations of an X-Ray Quasiperiodic Eruption Source
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Evidence for AGN Feedback in Galaxy Clusters and Groups
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
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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