Article snapshot taken from Wikipedia with creative commons attribution-sharealike license.
Give it a read and then ask your questions in the chat.
We can research this topic together.
NGC 4214 also has two older super star clusters, both with an age of 200 million years and respective masses of 2.6*10. and 1.5*10 solar masses.
Two satellites are known to exist around the vicinity of NGC 4214. One is DDO 113, which has an absolute V-band magnitude of −12.2. It stopped star formation around 1 billion years ago. Another, more recently discovered object is MADCASH-2, officially named MADCASH J121007+352635-dw. The name refers to the MADCASH (Magellanic Analog Dwarf Companions and Stellar Halos) project. It is similar to typical ultra-faint dwarf galaxies, with an absolute V-band magnitude of −9.15, except in that it shows evidence of multiple episodes of star formation in its recent past: one around 400 million years ago, and another 1.5 billion years ago.
One supernova has been observed in NGC 4214: SN 1954A (type Ib, mag. 9.8) was discovered by Paul Wild on 30 May 1954. In addition, the galaxy has hosted one luminous blue variable: SN 2010U (type LBV, mag. 16) was discovered by Kōichi Itagaki on 5 February 2010.
Ubeda, L.; Maíz-Apellániz, J.; MacKenty, J. W. (2004). H.J.G.L.M. Lamers; L.J. Smith; A. Nota (eds.). "Massive Young Star Clusters in NGC 4214". The Formation and Evolution of Massive Young Star Clusters, ASP Conference Series. 322: 221. Bibcode:2004ASPC..322..221U.
Hansen, Julie M. Vinter (4 June 1954). "Circular No. 1453". Central Bureau for Astronomical Telegrams. Observatory Copenhagen. Retrieved 27 November 2024.
"SN 1954A". Transient Name Server. IAU. Retrieved 27 November 2024.
"SN 2010U". Transient Name Server. IAU. Retrieved 27 November 2024.
Marion, G. H.; Vinko, J.; Wheeler, J. C.; Shetrone, M. (2010). "Supernova 2010U in NGC 4214". Central Bureau Electronic Telegrams. 2163: 1. Bibcode:2010CBET.2163....1M.