The 1992-93 dimming of FG Sagittae can be interpreted as a blue type R CrB decline. This favors the final flash scenario of the R CrB behavior and clears up the evolutionary connection between the planetary nebula nuclei and the R CrB phenomenon.
|Number of pages||5|
|Publication status||Published - Dec 1 1997|
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science