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astro-ph2000★ 187 cited

Accretion Disk Boundary Layers Around Neutron Stars: X-ray Production in Low-Mass X-ray Binaries

Robert Popham, Rashid Sunyaev

We present solutions for the structure of the boundary layer where the accretion disk meets the neutron star, which is expected to be the dominant source of high-energy radiation i…

astro-ph1998

Hyper-Accreting Black Holes and Gamma-Ray Bursts

Robert Popham, S. E. Woosley, Chris Fryer

A variety of current models for gamma-ray bursts (GRBs) suggest a common engine - a black hole of several solar masses accreting matter from a disk at a rate 0.01 to 10 solar masse…

astro-ph1998

Advection Dominated Accretion Flows in the Kerr Metric: II. Steady State Global Solutions

Robert Popham, Charles F. Gammie

In a previous paper we have written down equations describing steady-state, optically thin, advection-dominated accretion onto a Kerr black hole (Gammie and Popham 1997, hereafter…

astro-ph1997

Advection-Dominated Accretion Model of Sagittarius A*: Evidence for a Black Hole at the Galactic Center

Ramesh Narayan, Rohan Mahadevan, Jonathan E. Grindlay +2

Sgr A* at the Galactic Center is a puzzling source. It has a mass M=(2.5+/-0.4) x 10^6 solar masses which makes it an excellent black hole candidate. Observations of stellar winds…

astro-ph1997

Advection Dominated Accretion Flows in the Kerr Metric: I. Basic Equations

Charles F. Gammie, Robert Popham

We write down and solve equations describing steady state, optically thin, advection-dominated accretion onto a Kerr black hole. The mean flow, described by the relativistic fluid…

astro-ph1996

Heating of a Star by Disk Accretion

Robert Popham

We examine various ways in which disk accretion can heat an accreting star. These include 1) radiation emitted from the disk surface which is intercepted by the stellar surface, 2)…