Published February 24, 2026 | Version v1
Dataset Open

Is Mira B a low mass white dwarf?

Description

The data set contains  photometric observations in Johnson B and V bands of the short term variability (flickering) of Mira (omicron Ceti).
The observations were performed during 7 nights in the period August - October 2025, in the course of the last minimum of the Mira pulsations.

 

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