Search Results - "Yorke, H. W"
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Primordial star formation under the influence of far ultraviolet radiation: 1540 cosmological haloes and the stellar mass distribution
Published in Monthly notices of the Royal Astronomical Society (21-03-2015)“…We perform a large set of cosmological simulations of early structure formation and follow the formation and evolution of 1540 star-forming gas clouds to…”
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Formation of primordial supermassive stars by burst accretion
Published in Monthly notices of the Royal Astronomical Society (01-09-2015)“…Recent observations show that supermassive black holes (BHs) with ∼109 M⊙ exist at redshift z ≳ 6. A promising formation channel is the so-called direct…”
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Do lognormal column-density distributions in molecular clouds imply supersonic turbulence?
Published in Monthly notices of the Royal Astronomical Society (21-10-2010)“…Recent observations of column densities in molecular clouds find lognormal distributions with power-law high-density tails. These results are often interpreted…”
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ON THE SIMULTANEOUS EVOLUTION OF MASSIVE PROTOSTARS AND THEIR HOST CORES
Published in The Astrophysical journal (20-07-2013)“…Studies of the evolution of massive protostars and the evolution of their host molecular cloud cores are commonly treated as separate problems. However,…”
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Turbulent Mixing in the Outer Solar Nebula
Published in The Astrophysical journal (10-03-2006)“…The effects of turbulence on the mixing of gases and dust in the outer solar nebula are examined using three-dimensional MHD calculations in the shearing-box…”
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Supermassive star formation via episodic accretion: protostellar disc instability and radiative feedback efficiency
Published in Monthly notices of the Royal Astronomical Society (21-06-2016)“…The formation of supermassive stars (SMSs) is a potential pathway to seed supermassive black holes in the early universe. A critical issue for forming SMSs is…”
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2D Magnetohydrodynamics simulations of induced plasma dynamics in the near-core region of a galaxy cluster
Published in Monthly notices of the Royal Astronomical Society (01-02-2011)“…The mechanisms that maintain thermal balance in the intracluster medium (ICM) and produce the observed spatial distribution of the plasma density and…”
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Photon Bubbles in the Circumstellar Envelopes of Young Massive Stars
Published in The Astrophysical journal (20-06-2007)“…We show that the optically thick dusty envelopes surrounding young high-mass stars are subject to the photon bubble instability. The infrared radiation passing…”
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On the Surface Heating of Synchronously Spinning Short-Period Jovian Planets
Published in The Astrophysical journal (01-01-2005)“…We consider the atmospheric flow on short-period extrasolar planets through two-dimensional numerical simulations of hydrodynamics with radiation transfer. The…”
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Formation of primordial supermassive stars by burst accretion
Published 15-05-2015“…A promising formation channel of SMBHs at redshift 6 is the so-called DC model, which posits that a massive seed BH forms through gravitational collapse of a…”
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Massive stars and the energy balance of the interstellar medium. II. the 35 M⊙ star and a solution to the missing wind problem
Published in The Astrophysical journal (10-02-2006)“…We continue our numerical analysis of the morphological and energetic influence of massive stars on their ambient interstellar medium for a 35 M( star that…”
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Effect of OH depletion on measurements of the mass-to-flux ratio in molecular cloud cores
Published 25-08-2014“…The ratio of mass and magnetic flux determines the relative importance of magnetic and gravitational forces in the evolution of molecular clouds and their…”
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On the MHD structure of the solar tachocline. Steady and dynamical solutions
Published in New astronomy (01-12-1998)“…Using recent helioseismology measurements, we carry out a parameter study to investigate the steady and unsteady configurations of the solar tachocline…”
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On the Formation of Massive Stars
Published in The Astrophysical journal (20-04-2002)“…We calculate numerically the collapse of slowly rotating, nonmagnetic, massive molecular clumps of masses 30,60, and 120 Stellar Mass, which conceivably could…”
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Do lognormal column-density distributions in molecular clouds imply supersonic turbulence?
Published in Monthly notices of the Royal Astronomical Society (21-10-2010)Get full text
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Massive Stars and the Energy Balance of the Interstellar Medium. II. The 35 M sub( )Star and a Solution to the "Missing Wind Problem"
Published in The Astrophysical journal (10-02-2006)“…We continue our numerical analysis of the morphological and energetic influence of massive stars on their ambient interstellar medium for a 35 M sub( )star…”
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C$^+$ detection of warm dark gas in diffuse clouds
Published 19-07-2010“…We present the first results of the Herschel open time key program, Galactic Observations of Terahertz C$^+$ (GOT C+) survey of the [CII] fine-structure line…”
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Do Lognormal Column-Density Distributions in Molecular Clouds Imply Supersonic Turbulence?
Published 14-06-2010“…Recent observations of column densities in molecular clouds find lognormal distributions with power-law high-density tails. These results are often interpreted…”
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Journal Article