Compact symmetric objects and supermassive binary black holes in the VLBA Imaging and Polarimetry Survey

41Citations
Citations of this article
17Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

We present multifrequency Very Long Baseline Array (VLBA) follow-up observations of VLBA Imaging and Polarimetry Survey sources identified as likely compact symmetric objects (CSOs) or supermassive binary black holes (SBBHs). We also present new spectroscopic redshifts for 11 sources observed with the Hobby-Eberly Telescope. While no new SBBHs can be confirmed from these observations, we have identified 24 CSOs in the sample, 15 of which are newly designated, and refuted 52 candidates leaving 33 unconfirmed candidates. This is the first large uniform sample of CSOs which can be used to elicit some of the general properties of these sources, including morphological evolution and environmental interaction. We have detected polarized emission from two of these CSOs the properties of which are consistent with active galactic nuclei unification schemes.

Cite

CITATION STYLE

APA

Tremblay, S. E., Taylor, G. B., Ortiz, A. A., Tremblay, C. D., Helmboldt, J. F., & Romani, R. W. (2016). Compact symmetric objects and supermassive binary black holes in the VLBA Imaging and Polarimetry Survey. Monthly Notices of the Royal Astronomical Society, 459(1), 820–840. https://doi.org/10.1093/mnras/stw592

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free