NGC 4383 is a spiral galaxy located in the constellation Coma Berenices, within the Virgo Cluster. It was discovered on 23 May 1862 by Eduard Schönfeld.[2] It is one of the most H I-rich galaxies in the cluster, hosting a 6-kiloparsec (20,000 ly) bipolar outflow, travelling at an average velocity of 210 kilometres per second. The outflow was studied using the Multi-unit spectroscopic explorer (MUSE) at the Very Large Telescope (VLT).[3][4]

NGC 4383
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12h 25m 25.5s[1]
Declination16° 28′ 12″[1]
Redshift0.005704 ± 0.000010[1]
Group or clusterVirgo Cluster
Apparent magnitude (V)12.12[1]
Apparent magnitude (B)12.67[1]
Characteristics
TypeSA0/a[1]
Other designations
2MASX J12252551+1628120, UGC 7507, LEDA 40516, MCG +03-32-030, Mrk 769, SDSS J122525.52+162812.4[1]

References

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  1. ^ a b c d e f g "NGC 4383". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 26 April 2024.
  2. ^ "NGC 4383 (= PGC 40516)". cseligman. Retrieved 26 April 2024.
  3. ^ Cherevko, Vlad (23 April 2024). "Discovery in galaxy NGC 4383: Explosions eject a gas stream 20,000 light years away". Gagadget. Retrieved 26 April 2024.
  4. ^ Watts, Adam B.; Cortese, Luca; Catinella, Barbara; Fraser-McKelvie, Amelia; Emsellem, Eric; Coccato, Lodovico; van de Sande, Jesse; Brown, Toby H.; Ascasibar, Yago; Battisti, Andrew; Boselli, Alessandro; Davis, Timothy A.; Groves, Brent; Thater, Sabine (22 April 2024). "MAUVE: a 6 kpc bipolar outflow launched from NGC 4383, one of the most H I-rich galaxies in the Virgo cluster". Monthly Notices of the Royal Astronomical Society. 530 (2): 1968–1983. doi:10.1093/mnras/stae898. Retrieved 26 April 2024.