Zobrazeno 1 - 10
of 309
pro vyhledávání: '"Fürst, E."'
We present radio continuum and linear polarisation observations of the pulsar wind nebula CTB87 (G74.9+1.2) with the Effelsberg 100-m radio telescope between 4.75 and 32 GHz. An analysis of these new data including archived low-frequency observations
Externí odkaz:
http://arxiv.org/abs/2005.06125
Autor:
Manuchehri, Misha R., Fuerst, E. Pat, Guy, Stephen O., Shafii, Bahman, Pittmann, Dennis L., Burke, Ian C.
Publikováno v:
Weed Science, 2020 Nov 01. 68(6), 646-653.
Externí odkaz:
https://www.jstor.org/stable/27142982
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:
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
Many physical properties of this SNR such as spectrum and polarization can only be investigated by radio observations. The $\lambda$11 cm and $\lambda$6\ cm continuum and polarization observations of SNR G65.2+5.7 were made with the Effelsberg 100-m
Externí odkaz:
http://arxiv.org/abs/0904.3170
(Abridged) S147 is a large faint shell-type supernova remnant (SNR). Its remarkable spectral break at cm-wavelengths is an important physical property to characterize the SNR evolution. However, the spectral break is based on radio observations with
Externí odkaz:
http://arxiv.org/abs/0801.4803
Autor:
Carretti, E., Poppi, S., Reich, W., Reich, P., Fuerst, E., Bernardi, G., Cortiglioni, S., Sbarra, C.
Publikováno v:
Mon.Not.Roy.Astron.Soc.367:132-138,2006
Polarized diffuse emission observations at 1.4-GHz in a high Galactic latitude area of the northern Celestial hemisphere are presented. The 3.2 X 3.2 deg^2 field, centred at RA = 10h 58m, Dec = +42deg 18' (B1950), has Galactic coordinates l~172deg, b
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512286
Publikováno v:
Astron.Astrophys. 426 (2004) 909-924
We present a new sensitive 2675 MHz radio continuum map of the Cygnus Loop, which is used in conjunction with 408 MHz, 863 MHz and 1420 MHz maps from both the Effelsberg 100-m telescope and the DRAO Synthesis Telescope for a spectral analysis. Betwee
Externí odkaz:
http://arxiv.org/abs/astro-ph/0409176
The Cygnus Loop is classified as a middle-aged supernova remnant (SNR) located below the Galactic equator (l=74, b=-8.6) and 770 pc away from us. Its large size and little confusion with Galactic emission makes it an ideal test ground for evolutionar
Externí odkaz:
http://arxiv.org/abs/astro-ph/0205443
Publikováno v:
AIP Conf.Proc.609:3-8,2002
We report on sensitive 21cm and 11cm polarization surveys of the Galactic plane carried out with the Effelsberg 100-m telescope at arcmin angular resolution and some related work. Highly structured polarized emission is seen along the Galactic plane
Externí odkaz:
http://arxiv.org/abs/astro-ph/0111437