Draco Dwarf

The Draco Dwarf is one which has received specific attention.

The dark matter distribution within Draco Dwarf is at least nearly isothermal.

However, Draco Dwarf's narrow horizontal branch width does not support this model.

The Draco Dwarf contains primarily an old population of stars and insignificant amounts of interstellar matter (being basically dust free).

The Draco Dwarf is situated in the direction of the Draco Constellation at 34.6 above the galactic plane.

This suggests the need for further study of Draco Dwarf population's metallicity and ages and of dwarf spheroidals in general.

These include Carina Dwarf, Draco Dwarf, and Leo II Dwarf.

The central region of Draco Dwarf exhibits a concentration of more metal-rich stars there being more centrally concentrated red horizontal branch stars than blue horizontal branch stars.

Another is the Draco Dwarf Galaxy, one of the least luminous galaxies with an absolute magnitude of 8.6 and a diameter of only about 3,500 light years, discovered by Albert G. Wilson of Lowell Observatory in 1954.

The Draco Dwarf is a spheroidal galaxy which was discovered by Albert George Wilson of Lowell Observatory in 1954 on photographic plates of the National Geographic Society's Palomar Observatory Sky Survey (POSS).

Draco Dwarf contains many red giant branch (RGB) stars; five carbon stars have been identified in Draco Dwarf and four likely asymptotic giant branch (AGB) stars have been detected.