Results 121 to 130 of about 237,520 (386)
The Hard-to-soft Transition of GX 339–4 as Seen by Insight–HXMT
We present an analysis of the relativistic reflection spectra of GX 339–4 during the hard-to-soft transition of its 2021 outburst observed by Insight–HXMT.
Honghui Liu+8 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
Tidal Disruption of a Main-sequence Star by an Intermediate-mass Black Hole: A Bright Decade [PDF]
There has been suggestive evidence of intermediate-mass black holes (IMBHs; 103−5 M⊙) existing in some globular clusters (GCs) and dwarf galaxies, but IMBHs as a population remain elusive.
Jin-Hong Chen, R. Shen
semanticscholar +1 more source
Ozone‐based gas‐phase metal‐assisted chemical etching enables unprecedented room‐temperature fabrication of high‐quality silicon nanowires. The superior oxidation potential of O3 drives rapid vertical etching (1 µm min−1) while maintaining exceptional structural integrity. The pristine nanowire surfaces enable high‐performance core‐shell photodetectors
Hyein Cho+11 more
wiley +1 more source
Sowing the seeds of massive black holes in small galaxies: Young clusters as the building blocks of Ultra-Compact-Dwarf Galaxies [PDF]
Interacting galaxies often have complexes of hundreds of young stellar clusters of individual masses $\sim 10^{4-6}~M_\odot$ in regions that are a few hundred parsecs across.
Amaro-Seoane, Pau+4 more
core +3 more sources
Radial anisotropy in ω Cen limiting the room for an intermediate-mass black hole [PDF]
Finding an intermediate-mass black hole (IMBH) in a globular cluster (or proving its absence) would provide valuable insights into our understanding of galaxy formation and evolution.
A. Zocchi, M. Gieles, V. H'enault-Brunet
semanticscholar +1 more source
Intermediate Mass Black Holes in Star Clusters [PDF]
We have performed N-body simulations of the formation of intermediate mass black holes in young star clusters and the subsequent dynamical evolution of star clusters containing massive black holes. Our simulations show that runaway merging of massive main-sequence stars can produce an intermediate mass black hole in the M82 cluster MGG-11 if the ...
Holger Baumgardt, Junichiro Makino
openaire +2 more sources
Fast Neutron Detector Based on Hybrid 2D Perovskite Thin Films
This work presents the direct detection of fast neutrons using flexible hybrid 2D perovskite (PEA2PbBr4) thin‐film detectors. Thanks to their high low‐Z elements content and good charge transport, these materials enable efficient neutron detection. The thin film configuration allowed the operation at low voltage, and offer scalability, flexibility, and
Ilaria Fratelli+11 more
wiley +1 more source
The Maxwell invariant plays a fundamental role in the mathematical description of electromagnetic fields in charged spacetimes. In particular, it has recently been proved that spatially regular scalar fields which are non-minimally coupled to the Maxwell
Shahar Hod
doaj +1 more source
Intermediate-mass black hole growth and feedback in dwarf galaxies at high redshifts [PDF]
Intermediate-mass black holes (IMBHs; masses between $100\rm{\, and \,}10^{6} \, \mathrm{M}_{\odot }$) historically comprise of an elusive population compared to stellar-mass and supermassive black holes (BHs).
P. Barai, E. Pino
semanticscholar +1 more source