NGC 5765 explained

NGC 5765
Epoch:J2000
Constellation Name:Virgo
Z:0.027836
Dist Ly:~400 million ly
Type:Sy2
Appmag B:14.6
Names:MCG+01-38-004, MCG+01-38-005, IRAS 14483+0519, KPG 437, PSCz Q14483+0519, UGC 9554

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 400000000ly 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]

Notes and References

  1. NGC 5765. 25 November 2017.
  2. Web site: NGC 5765. Frommert. Hartmut. spider.seds.org. 2017-11-25.
  3. News: Hubble Image of the Week - MCG+01-38-004 and MCG+01-38-005. 2017-08-28. SciTech Daily. 2017-11-25. en-US.
  4. News: Hubble's Megamaser Galaxy. Hille. Karl. 2017-09-01. NASA. 2017-11-25. en.
  5. Web site: From microwaves to megamasers. www.spacetelescope.org. en-GB. 2017-11-25.