Astronomers discover how to feed a black hole
Date:
July 29, 2021
Source:
Instituto de Astrofi'sica de Canarias (IAC)
Summary:
Researchers have discovered long narrow dust filaments which
surround and feed black holes in the centers of galaxies, and
which could be the natural cause of the darkening of the centers
of many galaxies when their nuclear black holes are active.
FULL STORY ==========================================================================
The black holes at the centres of galaxies are the most mysterious objects
in the Universe, not only because of the huge quantities of material
within them, millions of times the mass of the Sun, but because of the incredibly dense concentration of matter in a volume no bigger than that
of our Solar System.
When they capture matter from their surroundings they become active,
and can send out enormous quantities of energy from the capture process, although it is not easy to detect the black hole during these capture
episodes, which are not frequent.
========================================================================== However, a study led by the researcher Almudena Prieto, of the Instituto
de Astrofi'sica de Canarias (IAC), has discovered long narrow dust
filaments which surround and feed these black holes in the centres of
galaxies, and which could be the natural cause of the darkening of the
centres of many galaxies when their nuclear black holes are active. The
results of this study have recently been published in the journal Monthly Notices of the Royal Astronomical Society (MNRAS).
Using images from the Hubble Space Telescope, the Very Large Telescope
(VLT) at the European Southern Observatory (ESO), and the Atacama Large Millimetre Array (ALMA) in Chile, the scientists have been able to obtain
a direct visualization of the process of nuclear feeding of a black hole
in the galaxy NGC 1566 by these filaments. The combined images show a
snapshot in which one can see how the dust filaments separate, and then
go directly towards the centre of the galaxy, where they circulate and
rotate in a spiral around the black hole before being swallowed by it.
"This group of telescopes has given us a completely new perspective of a supermassive black hole, thanks to the imaging at high angular resolution
and the panoramic visualization of its surroundings, because it lets
us follow the disappearance of the dust filaments as they fall into the
black hole," explains Almudena Prieto, the first author on the paper.
The study is the result of the long-term PARSEC project of the IAC,
which aims to understand how supermassive black holes wake up from their
long lives of hibernation, and after a process in which they accrete
material from their surroundings, they become the most powerful objects
in the Universe.
Part of this work was carried out within the Master's thesis in
Astrophysics of the University of La Laguna of Jakub Nadolny, carried
out at the IAC within the PARSEC project. Researchers Mar Mezcua and Juan
A. Ferna'ndez Ontiveros were also advisers to this work, while they had
PARSEC postdoctoral contracts at the IAC.
========================================================================== Story Source: Materials provided by Instituto_de_Astrofi'sica_de_Canarias_(IAC). Note: Content may be edited
for style and length.
========================================================================== Journal Reference:
1. M Almudena Prieto, Jakub Nadolny, Juan A Ferna'ndez-Ontiveros, Mar
Mezcua. Dust in the central parsecs of unobscured AGN: more
challenges to the torus. Monthly Notices of the Royal Astronomical
Society, 2021; 506 (1): 562 DOI: 10.1093/mnras/stab1704 ==========================================================================
Link to news story:
https://www.sciencedaily.com/releases/2021/07/210729143436.htm
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