Sub-parsec scale imaging of Centaurus A

At a distance of about 3.8 Mpc, the radio galaxy Centaurus A is the closest active galaxy. Therefore it is a key target for studying the innermost regions of active galactic nuclei (AGN). VLBI observations conducted within the framework of the TANAMI program enable us to study the central region of...

Full description

Bibliographic Details
Main Authors: Müller, Cornelia, Kadler, M., Ojha, R., Böck, M., Fromm, C. M., Ros, E., Rothschild, R. E., Wilms, J., team, TANAMI
Format: Report
Language:unknown
Published: arXiv 2010
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.1006.1486
https://arxiv.org/abs/1006.1486
id ftdatacite:10.48550/arxiv.1006.1486
record_format openpolar
spelling ftdatacite:10.48550/arxiv.1006.1486 2023-05-15T13:59:56+02:00 Sub-parsec scale imaging of Centaurus A Müller, Cornelia Kadler, M. Ojha, R. Böck, M. Fromm, C. M. Ros, E. Rothschild, R. E. Wilms, J. team, TANAMI 2010 https://dx.doi.org/10.48550/arxiv.1006.1486 https://arxiv.org/abs/1006.1486 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Astrophysics of Galaxies astro-ph.GA Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Preprint Article article CreativeWork 2010 ftdatacite https://doi.org/10.48550/arxiv.1006.1486 2022-04-01T14:18:11Z At a distance of about 3.8 Mpc, the radio galaxy Centaurus A is the closest active galaxy. Therefore it is a key target for studying the innermost regions of active galactic nuclei (AGN). VLBI observations conducted within the framework of the TANAMI program enable us to study the central region of the Cen A jet with some of the highest linear resolutions ever achieved in an AGN. This region is the likely origin of the gamma-ray emission recently detected by the Fermi Large Area Telescope (LAT). TANAMI monitors a sample of radio and gamma-ray selected extragalactic jets south of -30 degrees declination at 8.4 GHz and 22.3 GHz with the Australian Long Baseline Array (LBA) and the transoceanic antennas Hartebeesthoek in South Africa, the 6 m Transportable Integrated Geodetic Observatory (TIGO) in Chile and the 9 m German Antarctic Receiving Station (GARS) in O'Higgins, Antarctica. The highest angular resolution achieved at 8.4 GHz in the case of Cen A is 0.59mas x 0.978mas (natural weighting) corresponding to a linear scale of less than 18 milliparsec. We show images of the first three TANAMI 8.4 GHz observation epochs of the sub-parsec scale jet-counterjet system of Cen A. With a simultaneous 22.3 GHz observation in 2008 November, we present a high resolution spectral index map of the inner few milliarcseconds of the jet probing the putative emission region of gamma-ray-photons. : Proceedings of the Workshop "Fermi meets Jansky - AGN in Radio and Gamma-Rays", Savolainen, T., Ros, E., Porcas, R.W. & Zensus, J.A. (eds.), MPIfR, Bonn, June 21-23 2010 Report Antarc* Antarctic Antarctica DataCite Metadata Store (German National Library of Science and Technology) Antarctic
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics of Galaxies astro-ph.GA
Cosmology and Nongalactic Astrophysics astro-ph.CO
FOS Physical sciences
spellingShingle Astrophysics of Galaxies astro-ph.GA
Cosmology and Nongalactic Astrophysics astro-ph.CO
FOS Physical sciences
Müller, Cornelia
Kadler, M.
Ojha, R.
Böck, M.
Fromm, C. M.
Ros, E.
Rothschild, R. E.
Wilms, J.
team, TANAMI
Sub-parsec scale imaging of Centaurus A
topic_facet Astrophysics of Galaxies astro-ph.GA
Cosmology and Nongalactic Astrophysics astro-ph.CO
FOS Physical sciences
description At a distance of about 3.8 Mpc, the radio galaxy Centaurus A is the closest active galaxy. Therefore it is a key target for studying the innermost regions of active galactic nuclei (AGN). VLBI observations conducted within the framework of the TANAMI program enable us to study the central region of the Cen A jet with some of the highest linear resolutions ever achieved in an AGN. This region is the likely origin of the gamma-ray emission recently detected by the Fermi Large Area Telescope (LAT). TANAMI monitors a sample of radio and gamma-ray selected extragalactic jets south of -30 degrees declination at 8.4 GHz and 22.3 GHz with the Australian Long Baseline Array (LBA) and the transoceanic antennas Hartebeesthoek in South Africa, the 6 m Transportable Integrated Geodetic Observatory (TIGO) in Chile and the 9 m German Antarctic Receiving Station (GARS) in O'Higgins, Antarctica. The highest angular resolution achieved at 8.4 GHz in the case of Cen A is 0.59mas x 0.978mas (natural weighting) corresponding to a linear scale of less than 18 milliparsec. We show images of the first three TANAMI 8.4 GHz observation epochs of the sub-parsec scale jet-counterjet system of Cen A. With a simultaneous 22.3 GHz observation in 2008 November, we present a high resolution spectral index map of the inner few milliarcseconds of the jet probing the putative emission region of gamma-ray-photons. : Proceedings of the Workshop "Fermi meets Jansky - AGN in Radio and Gamma-Rays", Savolainen, T., Ros, E., Porcas, R.W. & Zensus, J.A. (eds.), MPIfR, Bonn, June 21-23 2010
format Report
author Müller, Cornelia
Kadler, M.
Ojha, R.
Böck, M.
Fromm, C. M.
Ros, E.
Rothschild, R. E.
Wilms, J.
team, TANAMI
author_facet Müller, Cornelia
Kadler, M.
Ojha, R.
Böck, M.
Fromm, C. M.
Ros, E.
Rothschild, R. E.
Wilms, J.
team, TANAMI
author_sort Müller, Cornelia
title Sub-parsec scale imaging of Centaurus A
title_short Sub-parsec scale imaging of Centaurus A
title_full Sub-parsec scale imaging of Centaurus A
title_fullStr Sub-parsec scale imaging of Centaurus A
title_full_unstemmed Sub-parsec scale imaging of Centaurus A
title_sort sub-parsec scale imaging of centaurus a
publisher arXiv
publishDate 2010
url https://dx.doi.org/10.48550/arxiv.1006.1486
https://arxiv.org/abs/1006.1486
geographic Antarctic
geographic_facet Antarctic
genre Antarc*
Antarctic
Antarctica
genre_facet Antarc*
Antarctic
Antarctica
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1006.1486
_version_ 1766268854799958016