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The effects of outbursts from Supermassive Black Holes: A close look at M87

Published online by Cambridge University Press:  29 March 2021

C. Jones Open the ORCID record for C. Jones [Opens in a new window]  and
W. Forman Open the ORCID record for W. Forman [Opens in a new window]
C. Jones
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden Street, Cambridge, MA, USA email: cjones@cfa.harvard.edu
W. Forman
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden Street, Cambridge, MA, USA email: cjones@cfa.harvard.edu
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Abstract

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Supermassive black holes (SMBHs) play[-105pt]Kindly check and confirm the Article Title. fundamental roles in the evolution of galaxies, groups, and clusters. The fossil record of supermassive black hole outbursts is seen through the cavities and shocks that are imprinted on these gas-rich systems. For M87, the central galaxy in the Virgo cluster, deep Chandra observations illustrate the physics of AGN feedback in hot, gas-rich atmospheres and allow measurements of the age, duration, and power of the outburst from the supermassive black hole in M87 that produced the observed cavities and shocks in the hot X-ray atmosphere.

Keywords

galaxies: elliptical and lenticularcDjetsevolutionX-rays: galaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 99 - 107
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

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