Further Evidence for a Supermassive Black Hole Mass-Pitch Angle Relation
We present new and stronger evidence for a previously reported relationship between galactic spiral arm pitch angle P (a measure of the tightness of spiral structure) and the mass M BH of a disk galaxy's nuclear supermassive black hole (SMBH). We use an improved method to accurately measure the spiral arm pitch angle in disk galaxies to generate
Berrier, J. C. et al.
Fecha de publicación:
6
2013