Dust changes in Sakurai's Object: new PAHs and SiC with coagulation of submicron-sized silicate dust into 10 µm-sized melilite grains (2021)
Attributed to:
Towards an understanding of astronomical silicate dust based on mineralogy, meteoritics and infrared spectroscopy
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stab1305
Publication URI: http://dx.doi.org/10.1093/mnras/stab1305
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1