CHANG-ES – XXVII. A radio/X-ray catalogue of compact sources in and around edge-on galaxies

Author:

Irwin Judith1ORCID,Dyer Jacqueline1,Drake Leonardo2,Wang Q Daniel2ORCID,Stil Jeroen3,Stein Yelena45,English Jayanne6,Wiegert Theresa1

Affiliation:

1. Department of Physics, Engineering Physics & Astronomy, Queens University , Kingston, ON K7L 3N6, Canada

2. Department of Astronomy, University of Massachusetts , LGRT-B 619E, 710 North Pleasant Street, Amherst, MA 01003-9305, USA

3. Department of Physics & Astronomy, University of Calgary , 834 Campus Place N. W., 2500 University Drive N W, Calgary, AB T2N 1N4, Canada

4. Faculty of Physics and Astronomy, Ruhr University Bochum , AIRUB D-44780, Germany

5. Observatoire Astronomique de Strasbourg, Université de Strasbourg, CNRS , UMR 7550, 11 rue de l’Université, F-67000 Strasbourg, France

6. Department of Physics and Astronomy, University of Manitoba , Winnipeg, MB R3T 2N2, Canada

Abstract

ABSTRACT We present catalogues of discrete, compact radio sources in and around the discs of 35 edge-on galaxies in the Continuum Halos in Nearby Galaxies – an EVLA Survey. The sources were extracted using the pybdsf program at both 1.6 GHz (L band) and 6.0 GHz (C band) from matching resolution (≈3 arcsec) data. We also present catalogues of X-ray sources from Chandra data sets for 27 of the galaxies. The sources at the two radio frequency bands were positionally cross-correlated with each other, and the result cross-correlated with the X-ray sources. All catalogues are included for download with this paper. We detect a total of 2507 sources at L band and 1413 sources at C band. 75 sources have been successfully cross-correlated in both radio bands plus X-ray. Three new nuclear sources are candidates for low luminosity active galactic nuclei in NGC 3877, NGC 4192, and NGC 5792; the one in NGC 3877 also appears to be variable. We also find new nuclear sources in two companion galaxies: NGC 4435 (companion to NGC 4438) and NGC 4298 (companion to NGC 4302). We have also discovered what appears to be a foreground double star; each star has X-ray emission and there is radio emission at both L band and C band in between them. This could be a colliding wind binary system. Suggestions for follow-up studies are offered.

Funder

Natural Sciences and Engineering Research Council of Canada

National Aeronautics and Space Administration

California Institute of Technology

National Science Foundation

Associated Universities, Inc.

European Space Agency

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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