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![Datei:M31, GS (nomenclature structures in the outer halo of the galaxy).jpg](http://upload.wikimedia.org/wikipedia/commons/thumb/0/00/M31%2C_GS_%28nomenclature_structures_in_the_outer_halo_of_the_galaxy%29.jpg/741px-M31%2C_GS_%28nomenclature_structures_in_the_outer_halo_of_the_galaxy%29.jpg)
Größe dieser Vorschau: 741 × 600 Pixel. Weitere Auflösungen: 297 × 240 Pixel | 593 × 480 Pixel | 949 × 768 Pixel | 1.266 × 1.024 Pixel | 2.531 × 2.048 Pixel | 4.816 × 3.897 Pixel
Originaldatei (4.816 × 3.897 Pixel, Dateigröße: 15,35 MB, MIME-Typ: image/jpeg)
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Version vom | Vorschaubild | Maße | Benutzer | Kommentar | |
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aktuell | 18:54, 6. Jun. 2020 | ![]() | 4.816 × 3.897 (15,35 MB) | Fabian RRRR | color for author's name changed |
23:19, 5. Jun. 2020 | ![]() | 4.816 × 3.897 (15,37 MB) | Fabian RRRR | passepartoutremoved | |
23:11, 5. Jun. 2020 | ![]() | 4.848 × 3.919 (9,9 MB) | Fabian RRRR | GSS -> GS | |
17:55, 5. Jun. 2020 | ![]() | 4.848 × 3.919 (9,49 MB) | Fabian RRRR | == {{int:filedesc}} == {{Information |Description=Andromeda [Ultra Deep 2019] Credit: Giuseppe Donatiello This image offers a good overview of the main structures on the disc and the external halo of Andromeda (M31). The disc appears quite regular and there is an abundant presence of young stars, gases and abundant dusts. The bulge is dominated by an older population. The external halo presents various irregularities and thickenings that we can consider as vestiges of dwarf galaxies incorpor... |
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