ISAAC spectrum of the centre of Centaurus A

Two wavelength regions of one of the infrared ISAAC spectra of the center of Centaurus A. The direction of the long spectrograph slit is vertical and the dispersion (wavelength) direction is horizontal; longer wavelengths are towards the right. The two emission lines shown originate in singly ionized Iron ([FeII]; rest wavelength 1256.68 nm) and in Hydrogen (Paschen-Beta; 1281.81 nm) and both are clearly tilted. This is due to the rapid rotation of the accretion disk surrounding the supermassive black hole in the center of the galaxy. The light from the receding edge of the disk is Doppler-shifted towards the red (to the right) and the light from the part of the disk approaching us is shifted to the left. This may be better seen in the inserted enlargements. Therefore the inclined disk shows a tilted spectrum. These motions may be represented in a rotation curve, cf. ESO Press Photo eso0109. There are other emitting areas above and below the nucleus, especially in the Paschen-Beta line. 

Credit:

ESO

Over de afbeelding

Id:eso0109b
Type:Observatie
Publicatiedatum:8 maart 2001
Gerelateerde berichten:eso0109
Grootte:2922 x 1797 px

Over het object

Naam:Centaurus A
Type:Local Universe : Galaxy
Local Universe : Galaxy : Component : Central Black Hole
Afstand:13 miljoen lichtjaren
Categorie:Galaxies
Quasars and Black Holes

Image Formats

Grote JPEG
1,8 MB

Wallpapers

1024x768
480,6 KB
1280x1024
699,2 KB
1600x1200
938,0 KB
1920x1200
1,1 MB
2048x1536
1,3 MB

Kleuren & filters

BandGolflengteTelescoop
Infrarood
Pa-beta
1.281 μmVery Large Telescope
ISAAC
Infrarood
FeII
1.256 μmVery Large Telescope
ISAAC