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Distance of Three Supernova Remnants from H I Line Observations in a Complex Region: G114.3+0.3, G116.5+1.1, and CTB 1 (G116.9+0.2)

  • Authors: Aylın Yar-Uyaniker, Bülent Uyaniker, and Roland Kothes

Yar‐Uyaniker, Uyaniker, & Kothes 2004 The Astrophysical Journal 616 247.

  • Provider: AAS Journals

Caption: Fig. 6.

Left: Averaged H I maps toward the SNRs CTB 1 and G116.5+1.1 showing the H I line emission averaged over velocity channels between ﹩v_{\mathrm{LSR}\,}=-15.5﹩ and −18.5 km s−1. The H I contours (in black) start from 10 K TB and run to 38 K TB in 7.0 K TB steps. Right: H I intensities averaged from ﹩v_{\mathrm{LSR}\,}=-27.5﹩ to −30.5 km s−1. Contour levels are 6–46 K TB with steps of 10 K TB. The 21 cm radio continuum emission in both images is overlaid as white contours at 6.0 and 7.0 K TB. The noise in the maps is 1.5 K TB because of the averaging of images over 3 km s−1.

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