Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP
E. Bortolas, E. Portaluri, E. Dalla Bonta', C. Arcidiacono, P. Severgnini, A. Gualandris
astro-ph.GA, astro-ph.IM
Submitted: 2026-06-30
Comments: 8 pages, part of the SHARP Science Book collection on New Astronomy (https://www.sciencedirect.com/special-issue/10W3B6JJBXH)
Journal ref: New Astronomy, Volume 128, 2026, 102593, ISSN 1384-1076 https://www.sciencedirect.com/science/article/pii/S138410762600076X
DOI: 10.1016/j.newast.2026.102593
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Science of the Einstein Telescope
- Astrophysics with the Laser Interferometer Space Antenna
- The influence of Massive Black Hole Binaries on the Morphology of Merger Remnants
- LISA Definition Study Report
- The Enhanced Resolution Imager and Spectrograph for the VLT
- Eight New Ultramassive Black Hole Masses confirm Best Correlation with Galaxy Core Sizes
- Galaxy Core Formation by Supermassive Black Hole Binaries: the Importance of Realistic Initial Conditions and Galaxy Morphology
- The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter and the early Universe
- The Merger Rates and Mass Assembly Histories of Dark Matter Haloes in the Two Millennium Simulations
- First Light for the GRAVITY+ Adaptive Optics: Extreme Adaptive Optics for the Very Large Telescope Interferometer
- Ejection of Supermassive Black Holes from Galaxy Cores
- Long-term evolution of massive black hole binaries. IV. Mergers of galaxies with collisionally relaxed nuclei
- The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope I. Overview of the instrument and its capabilities
- A dormant, overmassive black hole in the early Universe
- Core formation by binary scouring and gravitational wave recoil in massive elliptical galaxies
- A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars
- A black hole in a near-pristine galaxy 700 million years after the Big Bang
- Hypercompact Stellar Systems Around Recoiling Supermassive Black Holes
- Dynamical Friction in a Gaseous Medium
- Planck 2013 results. XVI. Cosmological parameters
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