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Draft:Sh2-29

From Wikipedia, the free encyclopedia


Sh2-29
Nebula
The nebula imaged by the OmegaCam on the VST
Observation data: J2000 epoch
Right ascension18h 10m 36s
Declination−23° 59′ 00″[1]
Distance~5,500 ly
ConstellationSagittarius
DesignationsSharpless 29
See also: Lists of nebulae

Sh2-29 is an emission nebula that is part of the Sharpless catalog. It is located in the constellation Sagittarius, near the Lagoon Nebula, and is approximately 5,500 light-years away from Earth.

Characteristics

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Star-forming region NGC 6559, imaged by the Danish 1.54-metre telescope. The "arc" caused by the binary system is visible within it.

Within the nebula, the star-forming region NGC 6559 stands out. Despite its small size of only a few light-years, it showcases the potential effects that stars have on nebulae. The brightest stars are no more than 2 million years old (compared to the 4.5 billion years of the Sun) and emit strong radiation that heats dust and gas, while stellar winds erode the surrounding area. One example is a cavity excavated by a very energetic binary system and kept expanding, creating an accumulation of interstellar material that forms a reddish arc-shaped rim. The diffuse reddish light originates from the emission of hydrogen gas, while the shimmering blue light comes from reflection by dust, along with filamentary clumps of dust that block light in small dark nebulae. All this makes Sh2-29 a potential target for research on star formation.[2]

References

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  1. ^ "LBN 29 -- HII (ionized) region". SIMBAD.
  2. ^ "Sboccia alla vista una culla stellare" [A star cradle blossoms into view]. media.inaf.it (in Italian). 13 December 2017.
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