Description by Sakib Rasool Towards the direction of Ursa Major in the sky, NGC 3077 is the unappreciated and forgotten third member of the M81 trio of galaxies along with M82. Another unusual aspect of this perturbed galaxy is the subtle blue core, which is surrounded by a disk consisting of an older stellar population. NGC 3077 is a smaller member of the M81 group, located 45' ESE of M81. Consisting of … Classed as a starburst dwarf galaxy, NGC 3077 is relatively nearby at 12 million light years. NGC-3077, SERVICE KIT, NGC, COOLING FAN. Consisting of chaotic and disordered structure, its appearance immediately hints at its turbulent history.
Signatures of star formation triggered by tidal interactions are present as the many HII regions interspersed within its structure and at least 36 separate HII regions have been catalogued. A series of tidally disrupted structures with striking blue stars is debris scattered from previous gravitational encounters with the other trio members, most notably M81. Use genuine … Normally it is the other way round, spiral galaxies consist of a golden core with blue spiral arms. Credit: NASA, ESA, J. Dalcanton and B. Williams (University of Washington) 304.1 KB Turbochef Genuine OEM replacement part.
The dark clumps of material scattered around the bright nucleus of NGC 3077 are pieces of wreckage from the galaxy's interactions with its larger neighbours. Optical images such as this one don't always show the full picture of the morphology and kinematics of galaxies and other instruments are utilised to detect different parts that belong to other areas of the electromagnetic spectrum. 3.2 MB The strange distribution of stellar matter is an indicator of a massive starburst of new stars being formed near the core due to the raw material of star formation being centrally concentrated at the nucleus.
A characteristic it has in common with M82 are multiple spidery tendrils of ionized hydrogen gas emanating outwards from its core. Witin the past few decades, the HI gas content of the M81 trio has been studied in superb detail and consists of many streamers and bridges connecting M81 and NGC 3077 together. 766.4 KB This structure has been nicknamed the "Garland" by professional astronomers and was first detected in photographic plates in the 1980's. NGC 3077 is a member of the M81 group of galaxies and it resides 12.5 million light-years from Earth.NASA, ESA, J. Dalcanton and B. Williams (University of Washington)
NGC 3077 is a member of the M81 group of galaxies and it resides 12.5 million light-years from Earth. These were first discovered in 1974.
A huge HI tail is also associated with NGC 3077 and contains more neutral gas than the core.
Observations with radio telescopes are able to map the distribution of neutral hydrogen gas (HI), which is invisible optically.
It looks like an elliptical galaxy, but is peculiar because of two reasons: First, it shows whispy edges and scattered dust clouds … Towards the direction of Ursa Major in the sky, NGC 3077 is the unappreciated and forgotten third member of the M81 trio of galaxies along with M82. Turbo chef provides commercial and residential ovens that set the industry standard for excellence.
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