NASA NTRS · 20010092688
Interfaces in N51D
Abstract
We obtained Far Ultraviolet Spectroscopic Explorer (FUSE) observations of four stars in the superbubble N51D in order to use the OVI interstellar absorption lines to study the interface between the hot (10(exp 6) K) interior gas and the surrounding warm (10(exp 4) K) dense shell.
Keep this discovery
Explore connections, maps & timelines
Chu, You-Hua, Wakker, Bart. 2001-09-11. Interfaces in N51D. https://ntrs.nasa.gov/citations/20010092688
Cite the original work for its findings. Save a collection to share your selection of sources.