Kinematics and stellar population of NGC 4486A
Context. NGC 4486A is a low-luminosity elliptical galaxy harbouring an edge-on nuclear disk of stars and dust. It is known to host a super-massive black hole. Aims: We study its large-scale kinematics and stellar population along the major axis to investigate the link between the nuclear and global properties. Methods: We use long-slit medium
Prugniel, Ph. et al.
Fecha de publicación:
4
2011