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Recoiling Black Holes: Electromagnetic Signatures, Candidates, and Astrophysical Implications
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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Data-driven Dynamics with Orbital Torus Imaging: A Flexible Model of the Vertical Phase Space of the Galaxy
Published 2025-01-01Get full text
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83
Relativistic Electron Acceleration and the “Ankle” Spectral Feature in Earth’s Magnetotail Reconnection
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84
A Study of the Star Clusters’ Population in the Giant Molecular Cloud G174+2.5
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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HCG 57: Evidence for Shock-heated Intergalactic Gas from X-Rays and Optical Emission Line Spectroscopy
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86
High-z Stellar Masses Can Be Recovered Robustly with JWST Photometry
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87
Investigations of MWISP Filaments. I. Filament Identification and Analysis Algorithms, and Source Catalog
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Introducing the Condor Array Telescope. V. Deep Broad- and Narrowband Imaging Observations of the M81 Group
Published 2025-01-01“…The images are characterized by an intricate web of faint, diffuse, continuum produced by starlight scattered from Galactic cirrus, and all prominent cirrus features identified in the broadband image can also be identified in the narrowband images. …”
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Discovery and Spectroscopic Confirmation of Aquarius III: A Low-mass Milky Way Satellite Galaxy
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Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER
Published 2025-01-01Get full text
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