Astronomy:NGC 4383
From HandWiki
| NGC 4383 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 25m 25.5s[1] |
| Declination | 16° 28′ 12″[1] |
| Redshift | Template:Plusminus[1] |
| Group or cluster | Virgo Cluster |
| Apparent magnitude (V) | 12.12[1] |
| Apparent magnitude (B) | 12.67[1] |
| Characteristics | |
| Type | SA0/a[1] |
| Other designations | |
| UGC 7507, MCG+03-32-030[1] | |
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]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 "NGC 4383". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+4383.
- ↑ "NGC 4383 (= PGC 40516)". https://cseligman.com/text/atlas/ngc43a.htm#4383. Retrieved 26 April 2024.
- ↑ Cherevko, Vlad (23 April 2024). "Discovery in galaxy NGC 4383: Explosions eject a gas stream 20,000 light years away". https://gagadget.com/en/443578-discovery-in-galaxy-ngc-4383-explosions-eject-a-gas-stream-20000-light-years-away/. Retrieved 26 April 2024.
- ↑ Watts, Adam B.; Cortese, Luca; Catinella, Barbara; Fraser-McKelvie, Amelia; Emsellem, Eric; Coccato, Lodovico; van de Sande, Jesse; Brown, Toby H. et al. (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. https://academic.oup.com/mnras/article/530/2/1968/7642869. Retrieved 26 April 2024.
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