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.



Sobre a imagem

Data de divulgação:8 de Março de 2001
Notícias relacionadas:eso0109
Tamanho:682 x 703 px

Sobre o objeto

Nome:Centaurus A, NGC 5128
Tipo:Local Universe : Galaxy : Component : Central Black Hole
Distância:13 milhão anos-luz
Quasars and Black Holes

Formatos de imagens

JPEG grande
58,7 KB


Veja também