Results 71 to 80 of about 205,282 (201)
Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network [PDF]
Gravitational-wave astronomy has been firmly established with the detection of gravitational waves from the merger of ten stellar-mass binary black holes and a neutron star binary.
Abbott, BP +99 more
core
Radiative properties and QPOs around charged black hole in Kalb–Ramond gravity
Studies of accretion disc luminosities and quasiperiodic oscillations around black holes may help us understand the gravitational properties of black hole spacetime.
Shokhzod Jumaniyozov +5 more
doaj +1 more source
We present dynamical models for the massive globular cluster G1. The goal is to measure or place a significant upper limit on the mass of any central black hole.
Bender R. +10 more
core +1 more source
A Tale of Two Black Holes: Multiband Gravitational-wave Measurement of Recoil Kicks
The nonlinear dynamics of General Relativity leave their imprint on remnants of black hole mergers in the form of a recoil “kick.” The kick has profound astrophysical implications across the black hole mass spectrum, from stellar-mass to supermassive ...
Shobhit Ranjan +4 more
doaj +1 more source
The GstLAL template bank for spinning compact binary mergers in the second observation run of Advanced LIGO and Virgo [PDF]
We describe the methods used to construct the aligned-spin template bank of gravitational waveforms used by the GstLAL-based inspiral pipeline to analyze data from the second observing run of Advanced LIGO and Virgo.
Blackburn, Kent +29 more
core +4 more sources
Spectrophotometric Reverberation Mapping of Intermediate-mass Black Hole NGC 4395
Understanding the origins of massive black hole seeds and their coevolution with their host galaxy requires studying intermediate-mass black holes (IMBHs) and estimating their mass.
Shivangi Pandey +10 more
doaj +1 more source
Intermediate Mass Black Hole Induced Quenching of Mass Segregation in Star Clusters [PDF]
In many theoretical scenarios it is expected that intermediate-mass black holes (IMBHs, with masses M ~ 100-10000 solar masses) reside at the centers of some globular clusters. However, observational evidence for their existence is limited.
Douglas Hamilton +8 more
core +1 more source
Optical Continuum Reverberation Mapping of a Candidate IMBH in a Nearby Seyfert 1 Galaxy
To investigate the short-term variability and determine the size of the optical continuum emitting region of intermediate-mass black holes (IMBHs), we carried out high-cadence, multiband photometric monitoring of a Seyfert 1 galaxy J0249−0815 across two ...
Wenwen Zuo +27 more
doaj +1 more source
We consider the possibility of detecting intermediate-mass ($10^3-10^4 M_{\odot}$) black holes, whose existence at the centers of globular clusters is expected from optical and infrared observations, using precise pulse arrival timing for the millisecond
Larchenkova, T. I., Lutovinov, A. A.
core +2 more sources
Constraints on metric-Palatini gravity from QPO data
In this work, we study metric-Palatini gravity extended by the antisymmetric part of the affine curvature. This gravity theory leads to general relativity plus a geometric Proca field.
Elham Ghorani +6 more
doaj +1 more source

