Results 11 to 20 of about 1,494,639 (351)

Overmassive Black Holes in Dwarf Galaxies Out to z ∼ 0.9 in the VIPERS Survey [PDF]

open access: yesThe Astrophysical Journal Letters, 2023
Supermassive black holes (SMBHs) are thought to originate from early universe seed black holes of mass M _BH ∼ 10 ^2 –10 ^5 M _⊙ and grown through cosmic time. Such seeds could be powering the active galactic nuclei (AGN) found in today’s dwarf galaxies.
Mar Mezcua   +5 more
doaj   +2 more sources

Cosmological physics with black holes (and possibly white dwarfs) [PDF]

open access: greenNew Astronomy Reviews, 2008
The notion that microparsec-scale black holes can be used to probe gigaparsec-scale physics may seem counterintuitive, at first. Yet, the gravitational observatory LISA will detect cosmologically-distant coalescing pairs of massive black holes, accurately measure their luminosity distance and help identify an electromagnetic counterpart or a host ...
Zoltan Haiman   +2 more
openaire   +4 more sources

Tidal Stripping of a White Dwarf by an Intermediate-mass Black Hole [PDF]

open access: yesThe Astrophysical Journal, 2023
Abstract During the inspiralling of a white dwarf (WD) into an intermediate-mass black hole (∼102−5 M ⊙), both gravitational waves (GWs) and electromagnetic (EM) radiation are emitted. Once the eccentric orbit’s pericenter radius approaches the tidal radius, the WD would be tidally stripped upon each ...
Jin-Hong 劲鸿 Chen 陈   +2 more
openaire   +4 more sources

The origins of off-centre massive black holes in dwarf galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2021
ABSTRACT Massive black holes often exist within dwarf galaxies, and both simulations and observations have shown that a substantial fraction of these may be off-centre with respect to their hosts. We trace the evolution of off-centre massive black holes (MBHs) in dwarf galaxies using cosmological hydrodynamical simulations, and show that
Jordan Van Nest   +12 more
openaire   +4 more sources

Tidal disruption of white dwarfs by intermediate mass black holes [PDF]

open access: diamondEPJ Web of Conferences, 2012
Modeling ultra-close encounters between a white dwarf and a spinning, intermediate mass black hole requires a full general relativistic treatment of gravity. This paper summarizes results from such a study.
Bode T.   +3 more
doaj   +2 more sources

Transmuted Gravity Wave Signals from Primordial Black Holes

open access: yesPhysics Letters B, 2018
Primordial black holes (PBHs) interacting with compact stars in binaries lead to a new class of gravity wave signatures that we explore. A small $10^{-16} - 10^{-7} M_{\odot}$ PBH captured by a neutron star or a white dwarf will eventually consume the ...
Takhistov, Volodymyr
core   +4 more sources

RNA N6‐methyladenosine modification suppresses replication of rice black streaked dwarf virus and is associated with virus persistence in its insect vector

open access: greenMolecular plant pathology, 2021
N6 methylation of adenosine (m6A) was recently discovered to play a role in regulating the life cycle of various viruses by modifying viral and host RNAs.
Shuping Tian   +3 more
semanticscholar   +3 more sources

Amino Acid Profiling and Chemometric Relations of Black Dwarf Honey and Bee Pollen. [PDF]

open access: yesFront Nutr, 2020
This research reports the characterization of bee pollen of Apis andreniformis colonies on the basis of morphology, proximate composition, the amino acid, and nutritive patterns in relation with their honey.
Sommano SR   +6 more
europepmc   +2 more sources

Multimessenger Signatures of Massive Black Holes in Dwarf Galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2018
Recent discoveries of massive black holes (MBHs) in dwarf galaxies suggest that they may have a more common presence than once thought. Systematic searches are revealing more candidates, but this process could be accelerated by predictions from simulations.
Jillian Bellovary   +9 more
openaire   +5 more sources

AT2018kzr: the merger of an oxygen–neon white dwarf and a neutron star or black hole [PDF]

open access: bronze, 2020
We present detailed spectroscopic analysis of the extraordinarily fast-evolving transient AT2018kzr. The transient's observed lightcurve showed a rapid decline rate, comparable to the kilonova AT2017gfo.
J. Gillanders, S. Sim, S. Smartt
semanticscholar   +3 more sources

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