- Spectroscopic properties of UV Ceti-type Stars
- UV Ceti-type flare stars have been generally carried out using photometric observations. However, high and Me-dwafs classified as flare stars (UV Ceti- type).
- 3-D Star Map of the 15 Nearest Stars - A NIAC Outreach Project
- UV Ceti B. Ross 248. Epsilon Eridani.
- FLARES OF STARS OF THE UV CETI TYPE
- FLARES OF STARS OF THE UV CETI TYPE. This article has been downloaded from IOPscience. Please scroll down to see the full text article.
- Six étoiles froides proches du Système solaire
- Elle s'intercale entre UV Ceti et Ross 154 dans la liste des systèmes stellaires les plus proches.
- Luyten 726-8 - Wikipedia, the free encyclopedia
- Like Luyten 726-8A, this star was also found to be variable and given the variable star designation UV Ceti.
- Luyten 726-8 AB / UV Ceti
- Star A and its companion UV Ceti have a combined mass of about 20 percent of Sol's but less than 11/100000th of its brightness.
- UV Ceti and the flare stars | AAVSO
- Jun 20, 2011 However, some of these stars belong to the spectacular class of variables known as the flare stars or the UV Ceti variables.
- UV Ceti star
- The flare activity is similar to that found on the Sun but appears comparatively more dramatic because of the normal faintness of red/orange dwarfs.
- Spectral Type M - UV Ceti
- Dayside of UV Ceti b. The dim sun will never set. Stars of type M are the weakest of all main sequence stars.
Uv Ceti is described in multiple online sources, as addition to our editors' articles, see section below for printable documents, Uv Ceti books and related discussion.
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