A high precision mass measurement of the central black hole in the massive elliptical galaxy NGC 2513 with ALMA molecular gas dynamics

Autor(en)

Shelley-Anne Harrisberg, Sabine Thater, Dieu D. Nguyen, Alvaro Hacar

Abstrakt

Supermassive black holes (SMBH) are believed to co-evolve with their host galaxies. Evidence for this co-evolution is found in the form of several correlations between the SMBH mass and various properties of the host galaxy, the tightest of which is the bulge stellar velocity dispersion. In order to better understand these correlations, a large and robust dataset of SMBH measurements is required, particularly in the low- and high-mass regime where measurements are still relatively few.

Organisation(en)

Institut für Astrophysik

Externe Organisation(en)

Université de Lyon

Seiten

1351

Anzahl der Seiten

1

Publikationsdatum

08-2024

ÖFOS 2012

103003 Astronomie, 103004 Astrophysik

Link zum Portal

https://ucrisportal.univie.ac.at/de/publications/7d7a5ca2-af5d-42ae-9b56-2361d5c0bbfa