VVV-WIT-07 is a variable star that was identified through the VVV (Vista Variables in the Via Lactea) survey. It belongs to the class of stars known as "WIT" stars, which are characterized by their variability. Specifically, VVV-WIT-07 is notable for its unusual behavior or characteristics, which have drawn the attention of astronomers. The VVV survey is aimed at studying the Milky Way's structure and stellar populations through infrared observations.
Articles by others on the same topic
There are currently no matching articles.