Stellar Dynamical Measurements of the Black Hole in M87 and Friends
APA
Gultekin, K. (2014). Stellar Dynamical Measurements of the Black Hole in M87 and Friends. Perimeter Institute. https://pirsa.org/14110077
MLA
Gultekin, Kayhan. Stellar Dynamical Measurements of the Black Hole in M87 and Friends. Perimeter Institute, Nov. 11, 2014, https://pirsa.org/14110077
BibTex
@misc{ pirsa_PIRSA:14110077, doi = {10.48660/14110077}, url = {https://pirsa.org/14110077}, author = {Gultekin, Kayhan}, keywords = {Strong Gravity}, language = {en}, title = {Stellar Dynamical Measurements of the Black Hole in M87 and Friends}, publisher = {Perimeter Institute}, year = {2014}, month = {nov}, note = {PIRSA:14110077 see, \url{https://pirsa.org}} }
University of Michigan–Ann Arbor
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Abstract
Stellar dynamical measurements of black hole masses have become the de facto standard method. I will give a brief review of how this measurement method works, along with arguments for its overall reliability and caveats. Then I will turn my attention to the case of the black hole in M87. The black hole is undeniably large ? billions of solar masses ? but has a stellar dynamical mass measurement in disagreement with gas dynamical mass measurements at about the 2 sigma level. I will discuss potential systematic uncertainties in both measurements and avenues to reconciling the discrepancy.