Evidence for cloud-to-cloud variations in the ratio of polarized thermal dust emission to starlight polarization

The correlation between optical starlight polarization and polarized thermal dust emission can be used to infer intrinsic dust properties. This correlation is quantified by the ratio RP/p, which has been measured by the Planck Collaboration to be 5.42 ± 0.05 MJy sr−1 at 353 GHz when averaged over la...

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Autors principals:	Mehandiratta N., Panopoulou G., Gjerløw E., Pelgrims V., Tassis K., Blinov D., Hensley B., Kypriotakis J. A., Maharana S., Mandarakas N., Pavlidou V., Potter S. B., Ramaprakash A. N., Skalidis R., Uppal N.
Format:	Artigo
Idioma:	Inglês
Publicat:	EDP Sciences 2026-04-01
Col·lecció:	Astronomy & Astrophysics
Matèries:	dust extinction ism: magnetic fields galaxy: general cosmic background radiation cosmology: observations
Accés en línia:	https://www.aanda.org/articles/aa/full_html/2026/04/aa57681-25/aa57681-25.html
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