CAOSP abstracts, Volume: 55, No.: 3, year: 2025

Abstract: RS Oph is one of the best studied recurrent novae, with its last outburst in 2021 triggering an extensive observational campaign across the whole electromagnetic spectrum, which led to the accumulation of an impressive amount of data. Here, we present the preliminary results of our analysis of interferometric data, which allowed us to provide insights into the structure and kinematics of the expanding nova shell.

Full text version of this article in PDF.


Back to:
CAOSP Vol. 55 No. 3 index
CAOSP archive main index
CAOSP main page
Astronomical Institute home page
Valid XHTML 1.0! Valid CSS!

Last update: April 29, 2025