activity
19982025
most citedThe Existence of Inner Cool Disks in the Low Hard State of Accreting Black Holes

112 citations · 853 across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.HE2025

Accretion geometry in neutron star low-mass X-ray binaries during the hard spectral state

Emmi Meyer-Hofmeister, Yilong Wang, B. F. Liu

We investigate the accretion geometry in neutron star low-mass X-ray binaries (LMXBs) in the hard spectral state. It is commonly accepted that, for low mass transfer rates, an adve…

astro-ph.HE2024★ 1 cited

A large population of neutron star low-mass X-ray binaries with long outburst recurrence time ?

E. Meyer-Hofmeister, Huaqing Cheng, B. F. Liu

Low-mass X-ray binaries (LMXBs) with neutron stars show quite different features which depend on the rate of mass transfer from the donor star. With a high transfer rate the Z sour…

astro-ph.HE2020★ 8 cited

Wind accretion in Cygnus X-1

Emmi Meyer-Hofmeister, B. F. Liu, E. Qiao +1

Context: Cygnus X-1 is a black hole X-ray binary system in which the black hole captures and accretes gas from the strong stellar wind emitted by its supergiant O9.7 companion star…

astro-ph.HE2018★ 9 cited

A Model for Spectral States and Their Transition in Cyg X-1

Ronald E. Taam, Erlin Qiao, B. F. Liu +1

A new accretion picture based on a small disk surrounding a black hole is developed for the wind-fed source Cyg X-1. The hard and soft spectral states of Cyg X-1 are interpreted in…

astro-ph.HE2017★ 12 cited

Interaction of the accretion flows in corona and disk near the black hole in AGN

E. Meyer-Hofmeister, B. F. Liu, E. Qiao

Accretion flows toward black holes can be of a quite different nature, described as an optically thick cool gas flow in a disk for high accretion rates or as a hot coronal opticall…

astro-ph.SR2015★ 30 cited

SU Uma stars: Rebrightenings after superoutburst

Friedrich Meyer, Emmi Meyer-Hofmeister

SU Uma stars after their long superoutbursts often show single or multiple rebrightenings. We show how this phenomenon can be understood as repeated reflections of transition waves…