Abstract
We present polarimetric observations of the Bok globule CB54 in the far-infrared via SOFIA/HAWC+ bands D (154 (Figure presented.) m) and E (214 (Figure presented.) m). We detect polarization with mean polarization degrees of (Figure presented.) (Figure presented.) 5.4 (Figure presented.) and (Figure presented.) (Figure presented.) 5.4 (Figure presented.) at 154 and 214 (Figure presented.) m, respectively. The polarization degree decreases toward the inner region of CB54, revealing a “polarization hole”. This finding can be explained by the impact of dichroic absorption counteracting the effect of polarized emission. The same effect allows us to explain the observed wavelength-dependent orientation of the linear polarization in the dense, central region of CB54. The polarization pattern appears uniform at core scales but un-ordered at larger scales—similar to what was found in previous studies of this object. The mean polarization angle amounts to (Figure presented.) = 62.4 (Figure presented.) 44.5° and (Figure presented.) = (Figure presented.) 60.0° at 154 and 214 (Figure presented.) m, respectively.
| Original language | English |
|---|---|
| Article number | e20220060 |
| Journal | Astronomische Nachrichten |
| Volume | 344 |
| Issue number | 5 |
| DOIs | |
| Publication status | Published - Jun 2023 |
| Externally published | Yes |
Keywords
- instrumentation: polarimeters
- ISM: magnetic fields
- polarization
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