A flocculent spiral galaxy is a type of spiral galaxy. Unlike the well-defined spiral architecture of a grand design spiral galaxy, flocculent (meaning "flaky") galaxies are patchy, with discontinuous spiral arms.[1] [2] Self-propagating star formation is the apparent explanation for the structure of flocculent spirals. Approximately 30% of spirals are flocculent, 10% are grand design, and the rest are referred to as "multi-armed".[3] The multiple-arm type is sometimes grouped into the flocculent category.[4]
The prototypical flocculent spiral is NGC 2841.[5]
Example | Class | Image | Constellation | Notes |
---|---|---|---|---|
NGC 1325 | SBbc | Eridanus | ||
NGC 1353 | SBb | Eridanus | ||
NGC 2775 | SA(r)ab | Cancer | [6] | |
NGC 2841 | SA(r)b | Ursa Major | ||
NGC 3521 | SAB(r s)bc | Leo | ||
NGC 4298 | SA(r s)c | Coma Berenices | ||
NGC 4414 | SA(r s)c | Coma Berenices | [7] | |
NGC 7793 | SA(s)d | Sculptor | ||
Sunflower Galaxy (Messier 63) | SAB(r s)cd | Canes Venatici | [8] | |