Early gray dust formation in the type IIn SN 2005ip
Ann-Sofie Bak Nielsen, Jens Hjorth, Christa Gall

TL;DR
This study investigates dust formation in supernova SN 2005ip, revealing early gray dust with high R_V values, indicating different dust properties than those in the Milky Way, based on modeling observed light curves.
Contribution
It provides the first detailed analysis of dust extinction properties in SN 2005ip, demonstrating early formation of gray dust with high R_V values through light curve modeling.
Findings
Dust formed about two months after explosion.
Extinction A_V increases up to 1 mag over 150 days.
R_V remains high (4.5–8), indicating gray dust.
Abstract
The physical characteristics of dust formed in supernovae is poorly known. In this paper, we investigate the extinction properties of dust formed in the type IIn SN 2005ip. The observed light curves of SN 2005ip all exhibit a sudden drop around 50 days after discovery. This has been attributed to dust formation in the dense circumstellar medium. We modeled the intrinsic light curves in six optical bands, adopting a theoretical model for the luminosity evolution of supernovae interacting with their circumstellar material. From the difference between the observed and intrinsic light curves, we calculated extinction curves as a function of time. The total-to-selective extinction ratio, , was determined from the extinction in the B and V bands. The resulting extinction, , increases monotonically up to about 1 mag, 150 days after discovery. The inferred value also increases…
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.
