activity
19982021
most citedA 1.4 GHz radio continuum and polarization survey at medium Galactic latitudes: II. First section

140 citations · 772 across the 13 of their papers we have counts for

collaborators
Showing astro-phShow all

10 papers · 1 filter

astro-ph2004★ 39 cited

Radio emission from the Cygnus Loop and its spectral characteristics

B. Uyaniker, W. Reich, A. Yar-Uyaniker +1

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 tele…

astro-ph2004★ 55 cited

Distance of three Supernova Remnants from HI line observations in a complex region: G114.3+0.3, G116.5+1.1, and CTB 1 (G116.9+0.2)

Aylin Yar-Uyaniker, Bulent Uyaniker, Roland Kothes

We present new radio continuum and HI images towards the supernova remnants (SNRs) G114.3+0.3, G116.5+1.1, and G116.9+0.2 (CTB 1) taken from the Canadian Galactic Plane Survey (CGP…

astro-ph2002★ 87 cited

Radio Polarization from the Galactic Plane in Cygnus

B. Uyaniker, T. L. Landecker, A. D. Gray +1

We present 1420 MHz (lambda=21cm) observations of polarized emission from an area of 117 degree square in the Galactic plane in Cygnus, covering 82 < l < 95, -3.5 < b < +5.5, a com…

astro-ph2002★ 51 cited

The distance to the SNR CTB109 deduced from its environment

Roland Kothes, Bulent Uyaniker, Aylin Yar

We conducted a study of the environment around the supernova remnant CTB109. We found that the SNR is part of a large complex of HII regions extending over an area of 400 pc along…

astro-ph2002★ 24 cited

A Highly Ordered Faraday-Rotation Structure in the Interstellar Medium

B. Uyaniker, T. L. Landecker

We describe a Faraday-rotation structure in the Interstellar Medium detected through polarimetric imaging at 1420 MHz from the Canadian Galactic Plane Survey (CGPS). The structure,…

astro-ph2002★ 8 cited

A large atomic hydrogen shell in the outer Galaxy: SNR or stellar wind bubble?

Bulent Uyaniker, Roland Kothes

We report the detection of a ring like HI structure toward l=90.0, b=2.8 with a velocity of v_LSR=-99 km/s. This velocity implies a distance of d=13 kpc, corresponding to a Galacto…