J2102+6015: a potential high-redshift multimessenger postprint

Author: Leonid I. Gurvits Sándor Frey Máté Krezinger Oleg Titov Tao An Yingkang Zhang Alexander G. Polnarev Krisztina É. Gabányi Krisztina Perger Alexey Melnikov
Submit Time:2023-02-19 20:58:59

Abstract: We present and briefly discuss results of several studies of the source J2102+6015 with tentatively defined redshift z=4:575 which demonstrates unusual properties in imaging and astrometric VLBI observations. Its properties might be considered as indications on the supermassive black hole binary which can be considered as a so far rare example of a high-redshift source of known electromagnetic and, possibly, predictable gravitational wave emissions.

Subject: Astronomy >> Astrophysical processes
Cite as: ChinaXiv:202303.02659 (or this version ChinaXiv:202303.02659V1)
DOI:10.12074/202303.02659V1
CSTR:32003.36.ChinaXiv.202303.02659.V1
TXID： 3f72ca9b-747e-406d-89c9-d25c1c76c848
Recommended references： Leonid I. Gurvits,Sándor Frey,Máté Krezinger,Oleg Titov,Tao An,Yingkang Zhang,Alexander G. Polnarev,Krisztina É. Gabányi,Krisztina Perger,Alexey Melnikov.J2102+6015: a potential high-redshift multimessenger.中国科学院科技论文预发布平台.[ChinaXiv:202303.02659V1] (Click&Copy)

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2023-02-19 20:58:59

ChinaXiv:202303.02659V1

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J2102+6015: a potential high-redshift multimessenger postprint

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