Catostomus bondi

Known as: Pantosteus bondi 
 
National Institutes of Health

Topic mentions per year

Topic mentions per year

1995-2016
024619952016

Papers overview

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2017
2017
Carbon-enhanced metal-poor stars (CEMP) are observed as a substantial fraction of the very metal-poor stars in the Galactic halo… (More)
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2012
2012
Accretion on to supermassive black holes (SMBHs) in galaxy formation simulations is frequently modelled by the Bondi–Hoyle… (More)
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2008
2008
The possibility that we live in a special place in the universe, close to the centre of a large void, seems an appealing… (More)
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2008
2008
Young stars orbiting in the gravitational potential well of forming star clusters may occasionally pass through associated dense… (More)
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2007
2007
Abstract In an earlier paper, we obtained exact solutions of the Wheeler–DeWitt equation for the Lemâıtre–Tolman–Bondi (LTB… (More)
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2005
2005
The Bondi-Hoyle formula gives the approximate accretion rate onto a point particle accreting from a uniform medium. However, in… (More)
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2004
2004
The classical Bondi-Hoyle formula gives the accretion rate onto a point particle of a gas with a uniform density and velocity… (More)
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2003
2003
We introduce a new computational method for embedding Lagrangian sink particles into an Eulerian calculation. Simulations of… (More)
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2001
2001
The relativistic jets in AGNs are probably driven by the action of supermassive, spinning black holes. There is very little… (More)
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1998
1998
In our program of studying numerically the so-called Bondi-Hoyle accretion in the fully relativistic regime, we present here… (More)
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