Benjamin Lee Davis

activity

20182021

most citedBlack Hole Mass Scaling Relations for Early-Type Galaxies:

M_{B H}

M_{*, s p h}

and

M_{B H}

M_{*, g a l}

117 citations · 174 across the 3 of their papers we have counts for

collaborators

Showing 2018Show all

3 papers · 1 filter

astro-ph.GA2018

Expected intermediate mass black holes in the Virgo cluster. II. Late-type galaxies

Alister W. Graham, Roberto Soria, Benjamin L. Davis

The Chandra X-ray Observatory's Cycle 18 Large Program titled "Spiral galaxies of the Virgo Cluster" will image 52 galaxies with the ACIS-S detector. Combined with archival data fo…

astro-ph.GA2018

Black Hole Mass Scaling Relations for Spiral Galaxies. II. $M_{BH}$ - $M_{, tot}$ and $M_{BH}$ - $M_{, disk}$

Benjamin L. Davis, Alister W. Graham, Ewan Cameron

Black hole mass ( $M_{B H}$ ) scaling relations are typically derived using the properties of a galaxy's bulge and samples dominated by (high-mass) early-type galaxies. Studying late-…

astro-ph.GA2018

Black Hole Mass Scaling Relations for Spiral Galaxies. I. $M_{BH}$ - $M_{*, sph}$

Benjamin L. Davis, Alister W. Graham, Ewan Cameron

The (supermassive black hole mass, $M_{BH}$ )-(bulge stellar mass, $M_{*, sph}$ ) relation is, obviously, derived using two quantities. We endeavor to provide accurate values…

Expected intermediate mass black holes in the Virgo cluster. II. Late-type galaxies

Black Hole Mass Scaling Relations for Spiral Galaxies. II. MBH​-M∗,tot​ and MBH​-M∗,disk​

Black Hole Mass Scaling Relations for Spiral Galaxies. I. MBH​-M∗,sph​

Black Hole Mass Scaling Relations for Spiral Galaxies. II. $M_{BH}$ - $M_{, tot}$ and $M_{BH}$ - $M_{, disk}$

Black Hole Mass Scaling Relations for Spiral Galaxies. I. $M_{BH}$ - $M_{*, sph}$