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Identifier 000402298
Title Study of the magnetic field and filamentary structures in the Polaris Flare molecular cloud
Alternative Title Μελέτη του μαγνητικού πεδίου και των νηματοειδών δομών στο μοριακό νέφος Polaris Flare.
Author Ψαραδάκη, Ιωάννα Δ.
Thesis advisor Τάσσης, Κωνσταντίνος
Abstract In diffuse molecular clouds, possible precursors of star-forming clouds, the effect of the magnetic field is unclear. In this thesis we compare the orientations of filamentary structures in the Polaris Flare, as seen through dust emission by Herschel, to the plane-of-the-sky magnetic field orientation (Bpos) as revealed by stellar optical polarimetry with RoboPol. Dust structures in this translucent cloud show a strong preference for alignment with Bpos. 70% of field orientations are consistent with those of the filaments (within 30o). We also explore the spatial variation of the relative orientations and find it to be uncorrelated with the dust emission intensity and correlated to the dispersion of polarization angles.
Language English
Subject Polarization
Structure
Αστρογέννεση
Μαγνητικά πεδία
Νηματοειδής δομές
Πόλωση
Issue date 2016-07-22
Collection   School/Department--School of Sciences and Engineering--Department of Physics--Post-graduate theses
  Type of Work--Post-graduate theses
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