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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. 5.

Averaged H I map toward the SNR G114.3+0.3. The H I line emission is averaged between ﹩v_{\mathrm{LSR}\,}=-4.8﹩ and −7.2 km s−1. The H I intensity contours (in black) start from 40 K TB up to 80 K TB with 10 K TB increasing steps. The 21 cm radio continuum emission is represented by white contours from 6.2 K TB and 6.6 K TB. The noise in the maps is 1.7 K TB because of the averaging of images.

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