Publication not explained

This publication has not yet been explained in plain language by the author(s). However, you can still read the publication.

If you are one of the authors, claim this publication so you can create a plain language summary to help more people find, understand and use it.

Featured Image

Read the Original

This page is a summary of: Constraining the parameters of the putative supermassive binary black hole in PG 1302–102 from its radio structure, Monthly Notices of the Royal Astronomical Society, October 2015, Oxford University Press (OUP),
DOI: 10.1093/mnras/stv2049.
You can read the full text:

Read

Contributors

The following have contributed to this page