Results 271 to 280 of about 43,779 (305)
Galaxy Tomography with the Gravitational Wave Background from Supermassive Black Hole Binaries
Chen Y.
europepmc +1 more source
Extended hot dust emission around the earliest massive quiescent galaxy
Ji Z +16 more
europepmc +1 more source
A binary merger product as the direct progenitor of a Type II-P supernova
Niu* Z +17 more
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures
Nature Astronomy, 2021While most of the compact-binary mergers detected by LIGO and Virgo are expected to consist of first-generation black holes formed from the collapse of stars, others might instead be of second (or higher) generation, containing the remnants of previous ...
D. Gerosa, M. Fishbach
semanticscholar +1 more source
Formation Channels of Single and Binary Stellar-Mass Black Holes
Handbook of Gravitational Wave Astronomy, 2021These are exciting times for binary black hole (BBH) research. LIGO and Virgo detections are progressively drawing a spectacular fresco of BBH masses, spins and merger rates.
M. Mapelli
semanticscholar +1 more source
2014
This chapter examines stellar-mass black holes. The empirical study of black holes began in the 1960s with the discovery of quasars and the advent of X-ray astronomy. X-ray detectors could detect X-rays coming from a particular direction—as the instrument rotated, the detector scanned the sky.
openaire +2 more sources
This chapter examines stellar-mass black holes. The empirical study of black holes began in the 1960s with the discovery of quasars and the advent of X-ray astronomy. X-ray detectors could detect X-rays coming from a particular direction—as the instrument rotated, the detector scanned the sky.
openaire +2 more sources
Stellar Mass Black Hole for Engineering Optimization
2017In recent years, nature-inspired algorithms have been popular due to the fact that many real-world optimization problems are increasingly large, complex and dynamic. By reasons of the size and complexity of the problems, it is necessary to develop an optimization method whose efficiency is measured by finding the near optimal solution within a ...
Premalatha Kandhasamy +2 more
openaire +1 more source
Stellar-Mass Black Hole Binaries as ULXs
AIP Conference Proceedings, 2005Ultraluminous X‐ray sources (ULXs) with Lx > 1039 ergs s−1 have been discovered in great numbers in external galaxies with ROSAT, Chandra, and XMM‐Newton. The central question regarding this important class of sources is whether they represent an extension in the luminosity function of binary X‐ray sources containing neutron stars and stellar‐mass ...
openaire +1 more source
Observational evidence for stellar mass black holes
Journal of Astrophysics and Astronomy, 1999I review the evidence for stellar mass black holes in the Galaxy. The unique properties of the soft X-ray transient (SXTs) have provided the first opportunity for detailed studies of the mass-losing star in low-mass X-ray binaries. The large mass functions of these systems imply that the compact object has a mass greater than the maximum mass of a ...
openaire +1 more source