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NGC 3506
Spiral galaxy in the constellation Leo / From Wikipedia, the free encyclopedia
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NGC 3506 is a spiral galaxy in the constellation Leo. It is located at a distance of circa 300 million light years from Earth, which, given its apparent dimensions, means that NGC 3506 is about 115,000 light years across. The galaxy has two main spiral arms, with high surface brightness, which can be traced for half a revolution before they fade. One arm splits into four spiral arcs.[2]
NGC 3506 | |
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![]() NGC 3506 by Hubble Space Telescope | |
Observation data (J2000 epoch) | |
Constellation | Leo |
Right ascension | 11h 03m 13.0s[1] |
Declination | 11° 04′ 36″[1] |
Redshift | 6408 ± 3 km/s[1] |
Distance | 297 Mly (86 Mpc)[1] |
Apparent magnitude (V) | 12.6 |
Characteristics | |
Type | Sc [1] |
Apparent size (V) | 1.2′ × 1.1′[1] |
Other designations | |
UGC 6120, MCG +02-28-047, PGC 33379[1] |
Three supernovae have been observed in NGC 3506: SN 2003L (type Ic, mag. 16.9),[3] SN 2017dfq (type Ia, mag. 15.3),[4] and SN 2021adgz (type II, mag. 19.4).[5] SN 2003L spectrum featured a relatively blue continuum, dominated by strong P-Cyg lines of Ca II (H and K) and Fe II and a relatively weaker Si II 635.5-nm line was also visible.[6]
It is an isolated galaxy.[7]