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On the origin of de-polarization in CB54

  • Niko Zielinski
  • , Sebastian Wolf
  • , Kate Pattle
  • University of Kiel
  • University College London

Research output: Contribution to a Journal (Peer & Non Peer)Articlepeer-review

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 languageEnglish
Article numbere20220060
JournalAstronomische Nachrichten
Volume344
Issue number5
DOIs
Publication statusPublished - Jun 2023
Externally publishedYes

Keywords

  • instrumentation: polarimeters
  • ISM: magnetic fields
  • polarization

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