Zobrazeno 1 - 10
of 2 478
pro vyhledávání: '"Wielebinski, R"'
The Sino-German 6cm polarization survey has mapped in total intensity and polarization intensity over an area of approximately 2200 square degrees in the Galactic disk. This survey provides an opportunity to search for Galactic supernova remnants (SN
Externí odkaz:
http://arxiv.org/abs/1304.4732
Autor:
Han, J. L., Gao, X. Y., Sun, X. H., Reich, W., Xiao, L., Reich, P., Xu, J. W., Shi, W. B., Fuerst, E., Wielebinski, R.
Publikováno v:
Proceedings of IAU Symp. 296, pp.202-209, 2014
We have observed 79 supernova remnants (SNRs) with the Urumqi 25m telescope at 6cm during the Sino-German 6cm polarization survey of the Galactic plane. We measured flux densities of SNRs at 6cm, some of which are the first ever measured or the measu
Externí odkaz:
http://arxiv.org/abs/1304.1949
Autor:
Han, J. L., Reich, W., Sun, X. H., Gao, X. Y., Xiao, L., Shi, W. B., Reich, P., Wielebinski, R.
We have finished the 6cm polarization survey of the Galactic plane using the Urumqi 25m radio telescope. It covers 10deg
Externí odkaz:
http://arxiv.org/abs/1202.1875
We present sub-mm continuum and heterodyne data of the interacting galaxy NGC 3627, obtained with the HHT and APEX. We find significant changes in the molecular line ratios over small scales in the southeastern part of this galaxy. The kinematics of
Externí odkaz:
http://arxiv.org/abs/1111.6071
Supernova remnants (SNRs) were often discovered in radio surveys of the Galactic plane. Because of the surface-brightness limit of previous surveys, more faint or confused SNRs await discovery. The Sino-German $\lambda$6\ cm Galactic plane survey is
Externí odkaz:
http://arxiv.org/abs/1107.0564
Autor:
Xiao, L., Han, J. L., Reich, W., Sun, X. H., Wielebinski, R., Reich, P., Shi, H., Lochner, O.
Linear polarization of diffuse Galactic emission is a signature of magnetic fields in the interstellar medium of our Galaxy. Observations at high frequencies are less affected by Faraday depolarization than those at lower frequencies and are able to
Externí odkaz:
http://arxiv.org/abs/1102.2978
(Abridged) We have conducted a total intensity and polarization survey of the Galactic plane at 6 cm using the Urumqi 25 m telescope for the Galactic longitude range of 10 deg
Externí odkaz:
http://arxiv.org/abs/1011.6425
Autor:
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.
Linearly polarized Galactic synchrotron emission provides valuable information about the properties of the Galactic magnetic field and the interstellar magneto-ionic medium, when Faraday rotation along the line of sight is properly taken into account
Externí odkaz:
http://arxiv.org/abs/1004.4072
Autor:
Landecker, T. L., Reich, W., Reid, R. I., Reich, P., Wolleben, M., Kothes, R., Uyaniker, B., Gray, A. D., Del Rizzo, D., Furst, E., Taylor, A. R., Wielebinski, R.
Context: Observations of polarized emission are a significant source of information on the magnetic field that pervades the Interstellar Medium of the Galaxy. Despite the acknowledged importance of the magnetic field in interstellar processes, our kn
Externí odkaz:
http://arxiv.org/abs/1004.2536
G156.2+5.7 is a large supernova remnant (SNR) first discovered in the ROSAT X-ray survey but radio observations are rare because of its low surface brightness and large size. Radio continuum and polarization images of the SNR G156.2+5.7 at lambda 6 c
Externí odkaz:
http://arxiv.org/abs/0705.2806