A new gravitational wave event reveals a binary black hole merger with total mass 190-265 solar masses, indicating black holes can form via gravitational-wave driven mergers beyond standard stellar channels.
Binary boson stars: Merger dynamics and formation of rotating remnant stars
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Visibility modulations from additional photon rings appear only in spherical boson stars at restricted inclinations, while rotating cases show incomplete rings.
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GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot}$
A new gravitational wave event reveals a binary black hole merger with total mass 190-265 solar masses, indicating black holes can form via gravitational-wave driven mergers beyond standard stellar channels.
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Ray tracing ultracompact boson stars: visibility modulations and incomplete photon rings
Visibility modulations from additional photon rings appear only in spherical boson stars at restricted inclinations, while rotating cases show incomplete rings.