Searching for the Kinematical Signature of a Black Hole in M87

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dc.creatorMerritt, David
dc.creatorOh, Siang Peng
dc.date1996-10-15
dc.date.accessioned2026-07-07T02:22:05Z
dc.date.available2026-07-07T02:22:05Z
dc.descriptionMany theories for the formation of massive black holes in galactic nuclei predict that the stellar motions should be anisotropic within the radius of influence of the black hole. We report tentative evidence for such an effect in M87.
dc.description2 Tex pages, 1 Postscript figure, uses stromlo.tex, epsf.sty. To appear in "The Nature of Elliptical Galaxies," Proceedings of the Second Stromlo Symposium, Eds. M. Arnaboldi, G. S. Da Costa & P. Saha
dc.identifierhttps://arxiv.org/abs/astro-ph/9610114
dc.identifierhttp://arxiv.org/abs/astro-ph/9610114
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10746
dc.subjectAstrophysics
dc.titleSearching for the Kinematical Signature of a Black Hole in M87
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