Testing New Ideas Regarding the Nature of Interstellar Extinction
David G. Turner, Daniel J. Majaess, David D. Balam

TL;DR
This paper challenges existing models of Galactic interstellar extinction by analyzing reddening parameters and diffuse interstellar bands, proposing a new extinction law that impacts our understanding of the universe's scale.
Contribution
It introduces a revised model of interstellar extinction based on new observational data, contradicting previous relations and suggesting a different wavelength dependence.
Findings
Identifies a minimum R_V=2.82 at X=0.83, indicating a new extinction law.
Shows inconsistencies with Cardelli et al. relations across multiple wavelengths.
Proposes that forward-scattered starlight affects observed extinction parameters.
Abstract
The nature of Galactic interstellar extinction is tested using reddening line parameters for several fields in conjunction with equivalent widths for the diffuse interstellar band at \AA. The Cardelli et al.relations [29] at infrared, optical, and ultraviolet wavelengths are inconsistent with the newly-derived quadratic variation of on reddening slope . A minimum of exists for , and is argued to represent true Galactic extinction described by . It matches expectations for a new description of extinction in the infrared, optical, and ultraviolet by Zagury [32]. Additional consequences, reddened stars with no 2175 \AAfeature and a correlation of normalized absorption with , are not predicted by the Cardelli et al.relation [29]. Known variations…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
