NGC 1409 | |
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Observation data (J2000 epoch) | |
Constellation | Taurus[1] |
Right ascension | 03h 41m 10.546s[2] |
Declination | −01° 18′ 10.12″[2] |
Heliocentric radial velocity | 7750±40 km/s[3] |
Apparent magnitude (V) | 15.4[3] |
Characteristics | |
Type | SB0[4] or SAB pec[3] |
Apparent size (V) | 1′.0 × 0′.8[3] |
Notable features | Interacting with NGC 1410 |
Other designations | |
NGC 1409, UGC 2821, PGC 13553[5][3] |
NGC 1409 is a quiescent[4] lenticular galaxy in the equatorial constellation of Taurus. It was discovered by the German-born astronomer William Herschel on January 6, 1785.[6] NGC 1409 is located in close proximity to the smaller Seyfert galaxy NGC 1410, and the two are strongly interacting. Their respective nuclei have a separation of just 23 kly, and they share a diffuse stellar envelope with a radius extending out to 49 kly.[4]
The morphological classification of this galaxy most closely matches type SB0, which indicates a barred lenticular galaxy. There is a conspicuous pipeline of dust and gas being funneled to NGC 1409 from NGC 1410. This lane has a typical width of 330 ly, passing to the north in front of NGC 1409 and then behind, becoming denser toward the galactic core. It has an estimated mass of 3×108 M☉ and is transferring mass at the estimated rate of 1.1–1.4 M☉ yr–1. However, there is no indications of recent star formation in NGC 1409 from this incoming material.[4]
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