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Introducing M 87

Blandford, Roger (1999) Introducing M 87. In: The Radio Galaxy Messier 87. Lecture Notes in Physics. No.530. Springer , Berlin, pp. 1-8. ISBN 978-3-540-66209-9. https://resolver.caltech.edu/CaltechAUTHORS:20190605-162311228

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Abstract

A brief introduction to the study of M 87 is presented. Attention is drawn to the surprisingly low bolometric power of the black hole. It is also argued that recent observations are quite constraining with respect to the origin of the jet power and the cause of its initial collimation. The bright jet knots provide a powerful diagnostic for constraining the character of jet flows as well as the properties of the ambient interstellar medium in the central few kpc of the nucleus. As it has been studied in such great detail throughout the electromagnetic spectrum, M 87 may have much to teach us about active galactic nuclei in general.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/BFb0106413DOIArticle
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ORCID:
AuthorORCID
Blandford, Roger0000-0002-1854-5506
Additional Information:© 1999 Springer-Verlag. I am indebted to Geoff Bicknell, Dan Harris, Klaus Meisenheimer, Fraser Owen and especially Hermann-Josef RSser for organising a timely and stimulating meeting and for travel support. I acknowledge NSF support under grant AST 95-29170.
Group:TAPIR
Funders:
Funding AgencyGrant Number
NSFAST 95-29170
Subject Keywords:Black Hole; Accretion Rate; Active Galactic Nucleus; Radio Galaxy; Massive Black Hole
Series Name:Lecture Notes in Physics
Issue or Number:530
Record Number:CaltechAUTHORS:20190605-162311228
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190605-162311228
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:96178
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:06 Jun 2019 03:02
Last Modified:08 May 2020 22:53

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