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- W2803599992 abstract "We revise the distance estimate to the supernova remnant (SNR) G109.1-1.0 (CTB 109) and its associated anomalous X-ray pulsar (AXP) 1E 2259+586 by re-analyzing both 408 and 1420 MHz continuum images, 21 cm HI absorption/emission spectra and $^{12}$CO emission spectra of CTB 109 and an adjacent compact HII region Sh 152, using the data from the Canadian Galactic Plane Survey. The HI images show that CTB 109 is morphologically located inside a shell in HI emission in the velocity range -61 to -70 km/s. Such a shell is likely blown by a stellar wind. The relation is supported by newly detected HI absorption features between $sim$ -61 km/s and -66 km/s, which are in the direction of the bright radio continuum emission within the north shell of CTB 109. We therefore give a distance of $sim$ 6 kpc to CTB 109, which is consistent with the distance of AXP 1E 2259+586 derived by the red clump stars method. The distance of $sim$ 6 kpc to the SNR/AXP system argues against a SNR/CO cloud interaction and instead favors a SNR/HI cloud interaction. The large distance argues for an anomalously large explosion energy which might be expected by a magnetar (AXP 1E 2259+586) harboring at the center of CTB 109." @default.
- W2803599992 created "2018-06-01" @default.
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- W2803599992 date "2007-11-15" @default.
- W2803599992 modified "2023-09-27" @default.
- W2803599992 title "The Distance of the SNR CTB 109/AXP 1E 2259+586:Is there a real interaction between CTB 109 and adjacent/adjoining clouds?" @default.
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