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Terme du glossaire : Galaxie lenticulaire

Description : Le mot lenticulaire est utilisé pour décrire les objets qui ont la forme d'une lentille. Les galaxies lenticulaires (S0 ou SB0) présentent des caractéristiques observationnelles proches des galaxies spirales et elliptiques. Les galaxies lenticulaires semblent avoir un disque et un bulbe central semblables à ceux des galaxies spirales, mais pas de bras spiraux perceptibles ; elles contiennent aussi principalement de très vieilles étoiles, comme celles qui dominent dans les galaxies elliptiques. Le processus de formation des galaxies lenticulaires fait encore l'objet de recherches, mais certains éléments indiquent qu'elles résultent de l'interaction entre des galaxies.

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The bright core of this galaxy is surrounded by a much fainter disk. This faint disk has thin dark rings.

The Lenticular Galaxy NGC 2787

Légende : The lenticular galaxy NGC 2787. This galaxy is a disk galaxy but lacks the large, dominant spiral arm structure seen in the disks of spiral galaxies. Its core is very bright compared to the core of a spiral galaxy. Thin rings of dust can be seen in the galaxy's disk.
Crédit : NASA/ESA and The Hubble Heritage Team Lien vers les crédits

License: CC-BY-4.0 Creative Commons (CC) Attribution 4.0 International (CC BY 4.0) Icônes

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The stars in Sextans take the shape of a hook with the concave part pointing south

Sextans Constellation Map

Légende : The constellation Sextans with its brighter stars and surrounding constellations. Sextans is surrounded by (going clockwise from the top): Leo, Hydra and Crater. Sextans is a small constellation with relatively few bright stars. Sextans spans the celestial equator and thus parts of the constellation are visible at some point in the year across the Earth. The whole constellation is visible in all but the most arctic and most antarctic regions. Sextans is best viewed in the evening in the northern hemisphere spring and southern hemisphere autumn. The lenticular galaxy NGC 3115 lies in Sextans. It is marked here with a red ellipse. The y-axis of this diagram is in degrees of declination with north as up and the x-axis is in hours of right ascension with east to the left. The sizes of the stars marked here relate to the star's apparent magnitude, a measure of its apparent brightness. The larger dots represent brighter stars. The Greek letters mark the brightest stars in the constellation. These are ranked by brightness with the brightest star being labeled alpha, the second brightest beta, etc., although this ordering is not always followed exactly. The dotted boundary lines mark the IAU's boundaries of the constellations and the solid green lines mark one of the common forms used to represent the figures of the constellations. The blue line at the top of the diagram marks the ecliptic. Neither the constellation boundaries, nor the lines joining the stars, nor the ecliptic, appear on the sky.
Crédit : Adapted by the IAU Office of Astronomy for Education from the original by the IAU and Sky & Telescope

License: CC-BY-4.0 Creative Commons (CC) Attribution 4.0 International (CC BY 4.0) Icônes