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Cited article:

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Molecular Clouds Associated with H ii Regions and Candidates within l = 106.°65 to 109.°50 and b = −1.°85 to 0.°95

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A Systematic Study of the Dust of Galactic Supernova Remnants. I. The Distance and the Extinction

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The Astrophysical Journal 891 (2) 137 (2020)
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A High Resolution Survey of the Galactic Plane at 408 MHz

A. K. Tung, R. Kothes, T. L. Landecker, J. Geisbüsch, D. Del Rizzo, A. R. Taylor, C. M. Brunt, A. D. Gray and S. M. Dougherty
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Astronomy & Astrophysics 597 A116 (2017)
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XMM-Newton and Canadian Galactic Plane Survey observations of the supernova remnant G107.5-1.5

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The search for faint radio supernova remnants in the outer Galaxy: five new discoveries

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G141.2+5.0, A NEW PULSAR WIND NEBULA DISCOVERED IN THE CYGNUS ARM OF THE MILKY WAY

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Distance to the SNR CTB109/AXP 1E 2259+586 by Hi absorption and self-absorption

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Revealing the Galactic HiiRegion G84.9+0.5 through 5 GHz Continuum and Polarization Emission and a Voigt Profile Analysis of Radio Recombination Line Observations

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