NGC 4217
| NGC 4217 | |
|---|---|
J2000 epoch) | |
| Constellation | Canes Venatici |
| Right ascension | 12h 15m 50.900s[1] |
| Declination | +47° 05′ 30.44″[1] |
| Redshift | 0.003419[2] |
| Heliocentric radial velocity | 1023 km/s[2] |
| Distance | 61.6 Mly (18.88 Mpc)[3] |
| Apparent magnitude (B) | 12.4[2] |
| Characteristics | |
| Type | Sb[4] |
| Other designations | |
| UGC 7282, MCG +08-22-087, PGC 39241[2] | |
NGC 4217 is an edge-on
).One supernova, SN 2022myz (type I, mag. 19), was discovered in NGC 4217 on 19 June 2022.[6]
Gallery
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Dust filamentsof NGC 4217. -
NGC 4217 by GALEX -
NGC 4217 (SDSS DR14)
References
- ^ S2CID 18913331.
- ^ a b c d "NGC 4217". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-12-12.
- S2CID 250737862. 50.
- ^ "Results for object NGC 4217 (NGC 4217)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2020-12-12.
- ^ "NGC 4217 is an edge-on spiral galaxy which lies approximately 60 million light years away in the constellation of Canes Venatici".
- ^ Transient Name Server entry for SN 2022myz. Retrieved 25 March 2023.
Further reading
- Thompson, Thomas W. J.; Howk, J. Christopher; Savage, Blair D. (2004). "Hubble Space Telescope Imaging of Extraplanar Dust Structures in the Edge-On Spiral NGC 4217". The Astronomical Journal. 128 (2): 662–673. doi:10.1086/422485.
External links
Media related to NGC 4217 at Wikimedia Commons
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