Seyfert Galaxy 3C120
Description
The active galaxy 3C120, located at about 450 million light-years near the Orion constelation, hosts a jet of particles with relativistic energies and velocities, observed here at radio wavelengths (1.3 cm) with the VLBA. The monthly sequence of images, starting in November 1997, shows the motion of several regions of enhanced energy moving in the plane of the sky at velocities of about 4-5 times that of the speed of light. Variability in the emission of these regions is interpreted as resulting from the interaction of the jet with "clouds" of material surrounding the central engine of the active galaxy. Thanks to the VLBA we can now make "movies" of these cosmic jets, by combining sequence of images of 3C120.
Creator
Legacy Astronomical Images
Rights
NRAO/AUI/NSF does not hold full copyright for this image. Contact the archivist for details.
Type
Legacy Astronomical Image
Object Name
3C120
Investigators
Jose-Luis Gomez et al.
Telescope
Very Long Baseline Array (VLBA)
Observation Date
1999-03-00
Type of Observation
continuum
Band
K
Wavelength
1.2 cm
Frequency
22 GHz
Center of Image
RA 4:33:11.100, Dec: 5:21:15.600 (J2000)
Field of View
0.000003 x 0.000001 degrees
Series
Active Galactic Nuclei Series
Unit
Seyferts Unit
Citation
Legacy Astronomical Images, “Seyfert Galaxy 3C120,” NRAO/AUI Archives, accessed December 24, 2024, https://www.nrao.edu/archives/items/show/33398.