Results 31 to 40 of about 1,324 (259)
The Astrophysical Journal, 2023 By using direct N -body numerical simulations, we model the dynamical coevolution of two supermassive black holes (SMBHs) and the surrounding stars in merging galaxies. In order to investigate how different stellar components evolve during the merger, we
Shuo Li +5 more
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Galaxies, 2023 We study radio and X-ray emissions from intermediate-mass black holes (IMBHs) and explore the unified model for accretion and ejection processes. The radio band survey of IMBH (candidate) hosted galaxies indicates that only a small fraction (∼0.6%) of ...
Xiaolong Yang, Jun Yang
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Masses of stellar black holes and testing theories of gravitation [PDF]
Astronomy Reports, 2003 11 pages, 2 ...
Postnov, K. A., Cherepashchuk, A. M.
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Investigating stellar-mass black hole kicks [PDF]
Monthly Notices of the Royal Astronomical Society, 2012 We investigate whether stellar-mass black holes have to receive natal kicks in order to explain the observed distribution of low-mass X-ray binaries containing black holes within our Galaxy. Such binaries are the product of binary evolution, where the massive primary has exploded forming a stellar-mass black hole, probably after a common envelope phase
Serena Repetto +2 more
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Searching for Stellar Mass Black Holes in the Solar Neighborhood [PDF]
The Astrophysical Journal, 1996 Latex, 7 pages, 3 postscript figures, submitted to ApJ Letters. Also available at http://fnas08.fnal.gov/
Heckler, Andrew F., Kolb, Edward W.
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Establishing a Relation between the Mass and the Spin of Stellar-Mass Black Holes [PDF]
Physical Review Letters, 2013 Stellar mass black holes (SMBHs), forming by the core collapse of very massive, rapidly rotating stars, are expected to exhibit a high density accretion disk around them developed from the spinning mantle of the collapsing star. A wide class of such disks, due to their high density and temperature, are effective emitters of neutrinos and hence called ...
Banerjee, Indrani +1 more
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Templates for stellar mass black holes falling into supermassive black holes [PDF]
Classical and Quantum Gravity, 2003 The spin modulated gravitational wave signals, which we shall call smirches, emitted by stellar mass black holes tumbling and inspiralling into massive black holes have extremely complicated shapes. Tracking these signals with the aid of pattern matching techniques, such as Wiener filtering, is likely to be computationally an impossible exercise.
Sathyaprakash, B., Schutz, B.
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Stellar Mass Black Hole Binaries as ULXs
, 2004 15 pages, 12 ...
Rappaport, S, Podsiadlowski, P, Pfahl, E
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FEBS Letters, EarlyView.We present robust protocols for the preparation of supported lipid bilayers (SLBs) incorporating either Salmonella smooth LPS or outer membrane vesicles (OMVs). We use a combination of quartz crystal microbalance with dissipation (QCM‐D) and fluorescence microscopy to both characterize the SLBs of various compositions and to probe their interactions ...
Hudson P. Pace +6 more
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Black Hole Accretion and Spin-up through Stellar Collisions in Dense Star Clusters
The Astrophysical JournalDynamical interactions in dense star clusters could significantly influence the properties of black holes, leaving imprints on their gravitational-wave signatures.
Fulya Kıroğlu +4 more
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