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Observations of the Local Group of Galaxies
PISCES DWARF / LGS3
From October 25
th to the 29
th 1978 a series of shmidt plates were taken in the area surrounding the galaxy M31 to try and locate some faint companions to that galaxy. After inspecting the plates 5 possible candidates were found. The LGS list was published in the IAU Circular 3305 by. Later examination of the 5 suspected galaxies revealed only one true member of the local group. The initial remarks from the plate examination said of LGS3
Resolved; Mag. 21 stars.
LGS3 is 3000 lightyears distant and is a satellite galaxy to M33. The galaxy has a diameter of 1700 lightyears.