List of nearby stellar associations and moving groups

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Star density maps of the Gaia Catalogue of Nearby Stars.The Sun is located at the centre of both maps. The regions with higher density of stars are shown; these correspond with known star clusters (Hyades and Coma Berenices) and moving groups. GCNS Poster Stellar Densities top image.png
Star density maps of the Gaia Catalogue of Nearby Stars.The Sun is located at the centre of both maps. The regions with higher density of stars are shown; these correspond with known star clusters (Hyades and Coma Berenices) and moving groups.

This is a list of nearby stellar associations and moving groups. A stellar association is a very loose star cluster, looser than an open cluster. A moving group is the remnant of such a stellar association. [1] Members of stellar associations and moving groups share similar kinematic properties, as well as similar ages and chemical composition.

The list (below) is sorted by the distance to the Solar System.

Main associations of the galactic plane in the night sky Sky Map 7 - Paper 29.png
Main associations of the galactic plane in the night sky

See also

Related Research Articles

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<span class="mw-page-title-main">Stellar kinematics</span> Study of the movement of stars

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<span class="mw-page-title-main">Taurus molecular cloud</span> Interstellar molecular cloud in the constellations Taurus and Auriga

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<span class="mw-page-title-main">SIMP J013656.5+093347</span> Possible exoplanet in the constellation Pisces

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<span class="mw-page-title-main">2MASS J21392676+0220226</span> Brown dwarf star in the constellation Aquarius

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<span class="mw-page-title-main">2MASS J03552337+1133437</span> Brown dwarf in the constellation Taurus

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<span class="mw-page-title-main">Tucana-Horologium association</span> Large stellar association

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<span class="mw-page-title-main">BD+29 5007</span> BD+29 5007 is a K-type star in the constellation Pegasus.

BD+29 5007 is a K-type star, located 77 light-years in the constellation Pegasus. It has a large-separation companion that was identified in 2016. The pair was identified to be a possible member of the 45+15
−5
million years old Argus association, though this is disputed.

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