Event horizon silhouette: implications to supermassive black holes in the galaxies M87 and Milky Way

DOI10.1007/S10714-019-2564-8zbMath1419.83035arXiv1903.09594OpenAlexW3105461764WikidataQ127674853 ScholiaQ127674853MaRDI QIDQ2003382

Vadim P. Smirnov, Natalia O. Nazarova, Vyacheslav I. Dokuchaev

Publication date: 8 July 2019

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1903.09594

zbMATH Keywords

black holesgeneral relativityevent horizongravitational lensing

Mathematics Subject Classification ID

Black holes (83C57) Galactic and stellar structure (85A15)

Related Items (2)

First analytical calculation of black hole shadow in McVittie metric ⋮ Modeling the motion of a bright spot in jets from black holes M87* and SgrA*

Cites Work

• Unnamed Item
• The Milky Way's supermassive black hole: how good a case is it? A challenge for astrophysics \& philosophy of science
• Spin and mass of the nearest supermassive black hole
• Maximal Analytic Extension of the Kerr Metric
• Global Structure of the Kerr Family of Gravitational Fields

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