Search Results - "SCHLEICHER, R"
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1
Blinks and saccades as indicators of fatigue in sleepiness warnings: looking tired?
Published in Ergonomics (01-07-2008)“…The present study examines changes in a variety of oculomotoric variables as a function of increasing sleepiness in 129 participants, who have been passed…”
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2
A New Jeans Resolution Criterion for (M)HD Simulations of Self-gravitating Gas: Application to Magnetic Field Amplification by Gravity-driven Turbulence
Published in The Astrophysical journal (10-04-2011)“…Cosmic structure formation is characterized by the complex interplay between gravity, turbulence, and magnetic fields. The processes by which gravitational…”
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3
The First Magnetic Fields
Published in Space science reviews (01-05-2012)“…We review current ideas on the origin of galactic and extragalactic magnetic fields. We begin by summarizing observations of magnetic fields at cosmological…”
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Journal Article Conference Proceeding -
4
Magnetic tension and instabilities in the Orion A integral-shaped filament
Published in Monthly notices of the Royal Astronomical Society (21-03-2018)“…Abstract The Orion nebula is a prime example of a massive star-forming region in our galaxy. Observations have shown that gravitational and magnetic energy are…”
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5
Formation of massive seed black holes via collisions and accretion
Published in Monthly notices of the Royal Astronomical Society (01-05-2018)“…Abstract Models aiming to explain the formation of massive black hole seeds, and in particular the direct collapse scenario, face substantial difficulties…”
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6
Role of Magnetic Fields in the Formation of Direct Collapse Black Holes
Published in The Astrophysical journal (01-03-2023)“…Direct collapse black holes are the leading candidates for the origin of the first supermassive black holes. However, the role of magnetic fields during their…”
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7
Magnetic Fields in the Large-Scale Structure of the Universe
Published in Space science reviews (01-05-2012)“…Magnetic fields appear to be ubiquitous in astrophysical environments. Their existence in the intracluster medium is established through observations of…”
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Journal Article Conference Proceeding -
8
Formation of supermassive black hole seeds in nuclear star clusters via gas accretion and runaway collisions
Published in Monthly notices of the Royal Astronomical Society (01-05-2021)“…ABSTRACT More than 200 supermassive black holes (SMBHs) of masses $\gtrsim 10^9\, \mathrm{M_{\odot }}$ have been discovered at z ≳ 6. One promising pathway for…”
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9
How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes
Published in Monthly notices of the Royal Astronomical Society (21-01-2015)“…Observations of high-redshift quasars at z > 6 indicate that they harbour supermassive black holes (SMBHs) of a billion solar masses. The direct collapse…”
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10
A detailed framework to incorporate dust in hydrodynamical simulations
Published in Monthly notices of the Royal Astronomical Society (01-04-2017)“…Dust plays a key role in the evolution of the interstellar medium and its correct modelling in numerical simulations is therefore fundamental. We present a new…”
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11
Magnetic field amplification during gravitational collapse - influence of turbulence, rotation and gravitational compression
Published in Monthly notices of the Royal Astronomical Society (01-07-2012)“…We study the influence of initial conditions on the magnetic field amplification during the collapse of a magnetized gas cloud. We focus on the dependence of…”
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12
The Role of Gas Fragmentation During the Formation of Supermassive Black Holes
Published in The Astrophysical journal (10-11-2019)“…We perform cosmological hydrodynamic simulations to study the effect of gas fragmentation on the formation of supermassive black hole seeds in the context of…”
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13
Magnetic Braking during Direct Collapse Black Hole Formation
Published in Astrophysical journal. Letters (01-07-2023)“…Magnetic fields are expected to be efficiently amplified during the formation of the first massive black holes via the small-scale dynamo and in the presence…”
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14
Formation of SMBH seeds in Population III star clusters through collisions: the importance of mass loss
Published in Monthly notices of the Royal Astronomical Society (01-04-2020)“…ABSTRACT Runaway collisions in dense clusters may lead to the formation of supermassive black hole (SMBH) seeds, and this process can be further enhanced by…”
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15
A mosquito salivary gland protein partially inhibits Plasmodium sporozoite cell traversal and transmission
Published in Nature communications (25-07-2018)“…The key step during the initiation of malaria is for motile Plasmodium parasites to exit the host dermis and infect the liver. During transmission, the…”
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16
The characteristic black hole mass resulting from direct collapse in the early Universe
Published in Monthly notices of the Royal Astronomical Society (21-12-2013)“…Black holes of a billion solar masses are observed in the infant Universe a few hundred million years after the big bang. The direct collapse of protogalactic…”
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17
The 3D Structure of CO Depletion in High-mass Prestellar Regions
Published in The Astrophysical journal (20-12-2019)“…Disentangling the different stages of the star formation process, in particular in the high-mass regime, is a challenge in astrophysics. Chemical clocks could…”
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18
Large-Scale Structure Formation: From the First Non-linear Objects to Massive Galaxy Clusters
Published in Space science reviews (01-05-2015)“…The large-scale structure of the Universe formed from initially small perturbations in the cosmic density field, leading to galaxy clusters with up to 10 15 M…”
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Turbulence and its connection to episodic accretion in binary YSOs
Published in Monthly notices of the Royal Astronomical Society (01-11-2021)“…ABSTRACT We report signatures of episodic accretion in young stellar objects (YSOs) that emerge in protobinary configurations in a gravoturbulent gas collapse…”
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The small-scale dynamo and the amplification of magnetic fields in massive primordial haloes
Published in Monthly notices of the Royal Astronomical Society (11-06-2013)“…While the present standard model of cosmology yields no clear prediction for the initial magnetic field strength, efficient dynamo action may compensate for…”
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