NGC 7793
A spiral galaxy in the constellation of Sculptor some 13 million light-years away from Earth. NGC 7793 is one of the brightest galaxies in the Sculptor Group, one of the closest groups of galaxies to the Local Group — the group of galaxies containing our galaxy, the Milky Way and the Magellanic Clouds.
Unlike some other spirals, NGC 7793 doesn’t have a very pronounced spiral structure, and its shape is further muddled by the mottled pattern of dark dust that stretches across the frame. Many bursts of bright pink can be seen in the galaxy, highlighting stellar nurseries containing newly forming baby stars.
Although it may look serene and beautiful from our perspective, this galaxy is actually a very dramatic and violent place.
Astronomers have discovered a powerful micro-quasar within NGC 7793 — a system containing a black hole actively feeding on material from a companion star. A micro-quasar is an object that has some of the properties of quasars in miniature. While many full-sized quasars are known at the cores of other galaxies, it is unusual to find a quasar in a galaxy’s disk rather than at its center.
Micro-quasars are almost like scale models — they allow astronomers to study quasars in detail. As material falls inwards towards this black hole, it creates a swirling disk around it. Some of the infalling gas is propelled violently outwards at extremely high speeds, creating jets streaking out into space in opposite directions. In the case of NGC 7793, these jets are incredibly powerful and are in the process of creating an expanding bubble of hot gas some 1,000 light-years across.
PlaneWave CDK24, Moravian C5, L600. LRGB-HA
SWOS- Mazlin,Parker,Forman,Hanson
Image Processing: Mark Hanson
Image Data and Calibration: Mark Hanson
Enjoy, Mark
With Ha Added
No Ha
Data Below from El Sauce, Chile 17” Planewave CDK LRGB - 450,300,300,300, Min each HA 300
