The Abell 85 BCG: a nucleated, core-less galaxy
arXiv:1603.00078 · doi:10.3847/0004-637X/819/1/50
Abstract
New high-resolution r band imaging of the brightest cluster galaxy (BCG) in Abell 85 (Holm 15A) was obtained using the Gemini Multi Object Spectrograph. These data were taken with the aim of deriving an accurate surface brightness profile of the BCG of Abell 85, in particular its central region. The new Gemini data show clear evidence of a previously unreported nuclear emission that is evident as a distinct light excess in the central kiloparsec of the surface brightness profile. We find that the light profile is never flat nor does it present a downward trend towards the center of the galaxy. That is, the new Gemini data show a different physical reality from the featureless, "evacuated core" recently claimed for the Abell 85 BCG. After trying different models, we find that the surface brightness profile of the BCG of Abell 85 is best fit by a double Sersic model.
Gemini web feature: Supermassive black hole that wasn't - http://gemini.edu/node/12477
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Cited by in corpus (11)
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- The buildup of the intracluster light of Abell 85 as seen by Subaru's Hyper Suprime-Cam
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- Ultramassive black holes in the most massive galaxies: versus
- Reading the tea leaves in the - and - diagrams: dry and gaseous mergers with remnant angular momentum
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