Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-29T16:31:43.190Z Has data issue: false hasContentIssue false
  • English
  • Français

Radio polarization observations of large supernova remnants at λ6 cm

Published online by Cambridge University Press:  29 January 2014

J. L. Han ,
X. Y. Gao ,
X. H. Sun ,
W. Reich ,
L. Xiao ,
P. Reich ,
J. W. Xu ,
W. B. Shi ,
E. Fürst  and
R. Wielebinski
J. L. Han
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Jia-20 Datun Road, Chaoyang District, Beijing 100012, China. [email protected]
X. Y. Gao
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Jia-20 Datun Road, Chaoyang District, Beijing 100012, China. [email protected]
X. H. Sun
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Jia-20 Datun Road, Chaoyang District, Beijing 100012, China. [email protected] Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
W. Reich
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
L. Xiao
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Jia-20 Datun Road, Chaoyang District, Beijing 100012, China. [email protected]
P. Reich
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
J. W. Xu
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Jia-20 Datun Road, Chaoyang District, Beijing 100012, China. [email protected]
W. B. Shi
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Jia-20 Datun Road, Chaoyang District, Beijing 100012, China. [email protected]
E. Fürst
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
R. Wielebinski
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have observed 79 supernova remnants (SNRs) with the Urumqi 25 m telescope at λ6 cm during the Sino-German λ6 cm polarization survey of the Galactic plane. We measured flux densities of SNRs at λ6 cm, some of which are the first ever measured or the measurements at the highest frequency, so that we can determine or improve spectra of SNRs. Our observations have ruled out spectral breaks or spectral flattening that were suggested for a few SNRs, and confirmed the spectral break of S147. By combining our λ6 cm maps with λ11 cm and λ21 cm maps from the Effelsberg 100 m telescope, we calculated the spectral index maps of several large SNRs. For many remnants we obtained for the first time polarization images, which show the intrinsic magnetic field structures at λ6 cm. We disapproved three objects as being SNRs, OA184, G192.8−1.1 and G16.8−1.1, which show a thermal spectrum and no polarization. We have discovered two large supernova remnants, G178.2−4.2 and G25.1−2.3., in the survey maps.

Keywords

supernova remnantspolarizationradio continuum: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S296: Supernova Environmental Impacts , January 2013 , pp. 202 - 209
Copyright
Copyright © International Astronomical Union 2014 

References

Foster, T., Kothes, R., Sun, X. H., Reich, W., & Han, J. L., 2006, A&A 454, 517Google Scholar
Foster, T., Cooper, B., Reich, W., Kothes, R., & West, J. 2013, A&A 549, A107Google Scholar
Fürst, E. & Reich, W. 2004, In: The magnetized Interstellar Medium, Uyaníker, B., Reich, W., and Wielebinski, R., ed., Copernicus GmbH, Katlenburg-Lindau, p. 141Google Scholar
Gao, X. Y. & Han, J. L. 2013, A&A 551, A16Google Scholar
Gao, X. Y., Han, J. L., Reich, W., Reich, P., Sun, X. H., & Xiao, L. 2011a, A&A 529, A159Google Scholar
Gao, X. Y., Reich, W., Han, J. L., Sun, X. H., Wielebinski, R., Shi, W. B., Xiao, L., Reich, P., Fürst, E., Chen, M. Z., & Ma, J. 2010, A&A 515, A64Google Scholar
Gao, X. Y., Sun, X. H., Han, J. L., Reich, W., Reich, P., & Wielebinski, R. 2011b, A&A 532, A144Google Scholar
Kundu, M. R. & Becker, R. H. 1972, AJ 77, 459CrossRefGoogle Scholar
Kundu, M. R., Angerhofer, P. E., Fürst, E., & Hirth, W. 1980, A&A 398, 993Google Scholar
Sofue, Y., Fürst, E., & Hirth, W. 1980, PASJ 32, 1Google Scholar
Shi, W. B., Han, J. L., Gao, X. Y., Sun, X. H., Xiao, L., Reich, P., & Reich, W. L. 2008, A&A 487, 601Google Scholar
Sun, X. H., Han, J. L., Reich, W., Reich, P., Shi, W. B., Wielebinski, R., & Fürst, E. 2007, A&A 463, 993Google Scholar
Sun, X. H., Reich, W., Han, J. L., Reich, P., & Wielebinski, R., 2006, A&A 447, 937Google Scholar
Sun, X. H., Reich, W., Han, J. L., Reich, P., Wielebinski, R., Wang, C., & Müller, P. 2011a, A&A 527, A74Google Scholar
Sun, X. H., Reich, P., Reich, W., Xiao, L., Gao, X. Y., & Han, J. L. 2011b, A&A 536, A83Google Scholar
Sun, X. H., Reich, W., Wang, C., Han, J. L., & Reich, P. 2011c, A&A 535, A64Google Scholar
Tian, W. W. & Leahy, D. 2006, A&A 447, 205Google Scholar
Urošević, D., Pannuti, T. G., & Leahy, D. 2007, ApJ 655, L41CrossRefGoogle Scholar
Uyaníker, B., Reich, W., Yar, A., Kothes, R., & Fürst, E. 2002, A&A 389, L61Google Scholar
Uyaníker, B., Reich, W., Yar, A., & Fürst, E. 2004, A&A 426, 909Google Scholar
Xiao, L., Fürst, E., Reich, W., & Han, J. L. 2008, A&A 482, 783Google Scholar
Xiao, L., Reich, W., Fürst, E., & Han, J. L. 2009, A&A 503, 827Google Scholar
Xiao, L., Han, J. L., Reich, W., Sun, X. H., Wielebinski, R., Reich, P., Shi, H., & Lochner, O. 2011, A&A 529, A15Google Scholar
Xu, J. W., Han, J. L., Sun, X. H., Reich, W., Xiao, L., Reich, P., & Wielebinski, R. 2007, A&A 470, 969Google Scholar