Reflection nebula | |
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emission nebula | |
NGC 6729 is the bright fan like nebula at the center of the image. | |
Observation data: J2000 epoch | |
Right ascension | 19 01 54.1 |
Declination | −36° 57′ 12″ |
Apparent dimensions (V) | 2.5′ × 2.0′ |
Constellation | Corona Australis |
Designations | Caldwell 68 |
See also: Lists of nebulae |
NGC 6729 (also known as Caldwell 68) is a reflection/emission nebula of the Corona Australis Molecular Cloud in the constellation Corona Australis. It was discovered by Johann Friedrich Julius Schmidt in 1861.
This fan-shaped nebula opens from the star R Coronae Australis toward the star T CrA to the south-east. R CrA is a pre-main-sequence star in the Corona Australis molecular complex, one of the closer star-forming regions of the galaxy at a distance of 130 pc. NGC 6729 is a variable nebula which shows irregular variations in brightness and in shape.
See also
- McNeil's Nebula
- NGC 1555 (Hind's Variable Nebula)
- NGC 2261 (Hubble's Variable Nebula)
References
- ^ "NGC/IC Project Database". Results for NGC 6729. Archived from the original on 2012-05-20. Retrieved 2010-12-09.
- "NASA/IPAC Extragalactic Database". Results for NGC 6729. Retrieved 2010-12-09.
- Robert Burnham, Jr.: Burnham's Celestial Handbook, Volume 2: Chamaeleon through Orion, pages 695-696: NGC 6726-6727-6729 and R Coronae Australis
External links
- [REDACTED] Media related to NGC 6729 at Wikimedia Commons
- NGC 6729 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Constellation of Corona Australis | |||||||||||
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Category |
New General Catalogue 6501 to 7000 | |
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Caldwell catalogue | |
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