Search Publications

Regulation of black-hole accretion by a disk wind during a violent outburst of V404 Cygni
DOI: 10.1038/nature17446 Bibcode: 2016Natur.534...75M

Ponti, G.; Charles, P. A.; Rodriguez, J. +7 more

Accretion of matter onto black holes is universally associated with strong radiative feedback and powerful outflows. In particular, black-hole transients have outflows whose properties are strongly coupled to those of the accretion flow. This includes X-ray winds of ionized material, expelled from the accretion disk encircling the black hole, and …

2016 Nature
INTEGRAL 117
Positron annihilation signatures associated with the outburst of the microquasar V404 Cygni
DOI: 10.1038/nature16978 Bibcode: 2016Natur.531..341S

Beloborodov, Andrei M.; Diehl, Roland; Greiner, Jochen +7 more

Microquasars are stellar-mass black holes accreting matter from a companion star and ejecting plasma jets at almost the speed of light. They are analogues of quasars that contain supermassive black holes of 106 to 1010 solar masses. Accretion in microquasars varies on much shorter timescales than in quasars and occasionally p…

2016 Nature
INTEGRAL 96
Repetitive patterns in rapid optical variations in the nearby black-hole binary V404 Cygni
DOI: 10.1038/nature16452 Bibcode: 2016Natur.529...54K

Ruiz, Javier; Enoto, Teruaki; Nogami, Daisaku +65 more

How black holes accrete surrounding matter is a fundamental yet unsolved question in astrophysics. It is generally believed that matter is absorbed into black holes via accretion disks, the state of which depends primarily on the mass-accretion rate. When this rate approaches the critical rate (the Eddington limit), thermal instability is supposed…

2016 Nature
INTEGRAL 77