Recoating Yepun's mirror
Rotation curve (velocity vrs. distance from the centre) of the disk surrounding the black hole at the centre of Centaurus A . From the ISAAC spectrum displayed in ESO Press Photo eso0109, the `average' gas velocities along the slit direction can be derived. Position `0' on the horizontal axis indicates the exact position of the galaxy nucleus; at the distance of Centaurus A, 1 arcsec corresponds to 55.5 light-years (17 pc). The blue triangles and the red squares correspond to emission lines from singly ionized Iron atoms ([Fe II]) and Hydrogen (Paschen-Beta), respectively. The high velocities are the hallmark of a central black hole. The thick solid line represents the expected velocities, assuming the presence of a 200 million solar-mass black hole at the centre.
Kilde:ESO
Om billedet
Id: | eso0109c |
Type: | Diagram |
Udgivelsesdato: | 8. marts 2001 |
Relaterede pressemeddelelser: | eso0109 |
Størrelse: | 682 x 703 px |
Om objektet
Navn: | Centaurus A, NGC 5128 |
Type: | Local Universe : Galaxy : Component : Central Black Hole |
Afstand: | 13 million lysår |
Kategori: | Galaxies Quasars and Black Holes |