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NGC 5765 
Summary
NGC 5765, also designated as MCG+01-38-004 and MCG+01-38-005,[1] is a pair of interacting megamasers in the constellation Virgo,[2] roughly 400,000,000 light-years (120,000,000 pc) away from Earth.[3] NGC 5765B is active, and energy is released from the core, some of which is absorbed by a nearby cloud of water. The cloud then re-emits this energy as microwaves.[4] These emissions were used to help redefine the Hubble constant.[5]
| NGC 5765 | |
|---|---|
 NGC 5765, seen from the Hubble Space Telescope. NGC 5765A is the upper galaxy, while NGC 5765B is the lower. | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 14h 50m 50.4s[1] |
| Declination | +05° 06′ 57″[1] |
| Redshift | 0.027836[1] |
| Distance | ~400 million ly |
| Apparent magnitude (B) | 14.6[1] |
| Characteristics | |
| Type | Sy2 |
| Other designations | |
| MCG+01-38-004, MCG+01-38-005, IRAS 14483+0519, KPG 437, PSCz Q14483+0519, UGC 9554 | |
References edit
- ^ a b c d e "NGC 5765". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 25 November 2017.
- ^ Frommert, Hartmut. "NGC 5765". spider.seds.org. Retrieved 2017-11-25.
- ^ "Hubble Image of the Week - MCG+01-38-004 and MCG+01-38-005". SciTech Daily. 2017-08-28. Retrieved 2017-11-25.
- ^ Hille, Karl (2017-09-01). "Hubble's Megamaser Galaxy". NASA. Retrieved 2017-11-25.
- ^ "From microwaves to megamasers". www.spacetelescope.org. Retrieved 2017-11-25.
External links edit
Media related to NGC 5765 at Wikimedia Commons- NGC 5765 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
