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On the need of an ultramassive black hole in OJ 287

On the need of an ultramassive black hole in OJ 287

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2847575042

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

The highly variable blazar OJ~287 is commonly discussed as an example of a binary black hole system. The 130 year long optical light curve is well explained by a model where the central body is a massive black hole of 18.35\(\times\)10\(^9\) solar mass that supports a thin accretion disc. The secondary black hole of 0.15\(\times\)10\(^9\) solar mas...

Alternative Titles

Full title

On the need of an ultramassive black hole in OJ 287

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2847575042

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2847575042

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2308.03017

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