At high Galactic latitudes, the Planck 353 GHz polarized dust emission is dominated by the Local Bubble shell at 200 to 300 pc from the Sun.
G., Lazarian , A., & Vaillancourt , J
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Local Bubble contribution to the 353-GHz dust polarized emission
At high Galactic latitudes, the Planck 353 GHz polarized dust emission is dominated by the Local Bubble shell at 200 to 300 pc from the Sun.