SwePub
Sök i LIBRIS databas

  Utökad sökning

WFRF:(Abramowicz Marek A 1945)
 

Sökning: WFRF:(Abramowicz Marek A 1945) > (2015-2019) > A magnetized torus ...

A magnetized torus for modeling Sagittarius A* millimeter images and spectra

Vincent, F. H. (författare)
Yan, W. (författare)
Straub, O. (författare)
visa fler...
Zdziarski, A. A. (författare)
Abramowicz, Marek A, 1945 (författare)
Gothenburg University,Göteborgs universitet,Institutionen för fysik (GU),Department of Physics (GU)
visa färre...
 (creator_code:org_t)
2015-01-22
2015
Engelska.
Ingår i: Astronomy & Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 574
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • Context. The supermassive black hole, Sagittarius (Sgr) A*, in the centre of our Galaxy has the largest angular size in the sky among all astrophysical black holes. Its shadow, assuming no rotation, spans similar to 50 mu as. Resolving such dimensions has long been out of reach for astronomical instruments until a new generation of interferometers being operational during this decade. Of particular interest is the Event Horizon Telescope (EHT) with resolution similar to 20 mu as in the millimeter- wavelength range 0.87 mm- 1.3 mm. Aims. We investigate the ability of the fully general relativistic Komissarov (2006, MNRAS, 368, 993) analytical magnetized torus model to account for observable constraints at Sgr A* in the centimeter and millimeter domains. The impact of the magnetic field geometry on the observables is also studied. Methods. We calculate ray-traced centimeter- and millimeter-wavelength synchrotron spectra and images of a magnetized accretion torus surrounding the central black hole in Sgr A*. We assume stationarity, axial symmetry, constant specific angular momentum and polytropic equation of state. A hybrid population of thermal and non-thermal electrons is considered. Results. We show that the torus model is capable of reproducing spectral constraints in the millimeter domain, and in particular in the observable domain of the EHT. However, the torus model is not yet able to fit the centimeter spectrum. 1.3 mm images at high inclinations are in agreement with observable constraints. Conclusions. The ability of the torus model to account for observations of Sgr A* in the millimeter domain is interesting in the perspective of the future EHT. Such an analytical model allows very fast computations. It will thus be a suitable test bed for investigating large domains of physical parameters, as well as non-black-hole compact object candidates and alternative theories of gravity.

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Nyckelord

Galaxy: center
accretion
accretion disks
black hole physics
relativistic processes
SUPERMASSIVE BLACK-HOLE
HOT ACCRETION FLOWS
GALACTIC-CENTER
SYNCHROTRON-RADIATION
MHD SIMULATIONS
STELLAR ORBITS
SCALE JET
POLARIZATION
TELESCOPE
EMISSION
Astronomy & Astrophysics

Publikations- och innehållstyp

ref (ämneskategori)
art (ämneskategori)

Hitta via bibliotek

Till lärosätets databas

Hitta mer i SwePub

Av författaren/redakt...
Vincent, F. H.
Yan, W.
Straub, O.
Zdziarski, A. A.
Abramowicz, Mare ...
Om ämnet
NATURVETENSKAP
NATURVETENSKAP
och Fysik
och Astronomi astrof ...
Artiklar i publikationen
Astronomy & Astr ...
Av lärosätet
Göteborgs universitet

Sök utanför SwePub

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Stäng

Kopiera och spara länken för att återkomma till aktuell vy