What can ISM and non-photospheric highly ionised lines in white dwarf spectra reveal about the ß CMa tunnel? (2020)
Attributed to:
Rolling Grant Programme in Astrophysics, Planetary Science and Space Instrumentation - 2007-2012
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1017/s1743921320001374
Publication URI: http://dx.doi.org/10.1017/s1743921320001374
Type: Journal Article/Review
Parent Publication: Proceedings of the International Astronomical Union
Issue: S357