NGC 6334, colloquially known as the Cat's Paw Nebula, or Gum 64, is an emission nebula and star-forming region located in the constellation Scorpius.[4] NGC 6334 was discovered by astronomer John Herschel in 1837, who observed it from the Cape of Good Hope in South Africa.[5] The nebula is located in the Carina–Sagittarius Arm of the Milky Way,[6] at a distance of approximately 5.5 kilolight-years from the Sun.[7]
Emission nebula | |
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Observation data: J2000 epoch | |
Right ascension | 17h 20m 50.9s[1] |
Declination | −36° 06′ 54″[1] |
Distance | 4.37 ± 0.65 kly (1.34 ± 0.2 kpc)[2] ly |
Apparent dimensions (V) | 40'×23' |
Constellation | Scorpius |
Physical characteristics | |
Radius | 40 ly |
Designations | NGC 6334, ESO 392-EN 009,[3] Sharpless 8, RCW 127, Gum 64 |
The nebula is a high mass filamentary cloud structure spanning ~320 ly. In the visible part of the spectrum, it emits mainly in red (from hydrogen atoms) and blue (from oxygen atoms).[8] Several embedded star-forming regions have been identified from infrared and radio emissions. Four of these sites have formed H II regions.[6]
Gallery
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Spitzer view of the star-forming region NGC 6334
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This portrait of NGC 6334 was created from images taken with the Wide Field Imager instrument at the 2.2-metre MPG/ESO telescope at the La Silla Observatory in Chile.
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Submillimetre views of the star formation region
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Protocluster NGC 6334I is a star-forming cloud in the Cat's Paw Nebula.[10]
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The photograph of NGC 6334.
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VISTA infrared view of NGC 6334.
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NGC 6334 photographed in 1986
See also
editReferences
edit- ^ a b Kharchenko, N. V.; et al. (2013), "Global survey of star clusters in the Milky Way. II. The catalogue of basic parameters", Astronomy and Astrophysics, 558: 8, arXiv:1308.5822, Bibcode:2013A&A...558A..53K, doi:10.1051/0004-6361/201322302, S2CID 118548517, A53.
- ^ Reid, M. J.; Menten, K. M.; Brunthaler, A.; Zheng, X. W.; Dame, T. M.; Xu, Y.; Wu, Y.; Zhang, B.; Sanna, A.; Sato, M.; Hachisuka, K.; Choi, Y. K.; Immer, K.; Moscadelli, L.; Rygl, K. L. J.; Bartkiewicz, A. (2014). "Trigonometric Parallaxes of High Mass Star Forming Regions: The Structure and Kinematics of the Milky Way". The Astrophysical Journal. 783 (2): 130. arXiv:1401.5377. Bibcode:2014ApJ...783..130R. doi:10.1088/0004-637X/783/2/130.
- ^ "NGC 6334". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2007-04-10.
- ^ Nemiroff, R.; Bonnell, J., eds. (2003-07-17). "The Cat's Paw Nebula". Astronomy Picture of the Day. NASA. Retrieved 2007-11-05.
- ^ "NGC 6334 - The Cat's Paw Nebula". SEDS Database. SEDS. Retrieved 2008-04-15.
- ^ a b Sadaghiani, M.; et al. (March 2020). "Physical properties of the star-forming clusters in NGC 6334. A study of the continuum dust emission with ALMA". Astronomy & Astrophysics. 635: 25. arXiv:1911.06579. Bibcode:2020A&A...635A...2S. doi:10.1051/0004-6361/201935699. S2CID 208077028. A2.
- ^ Russeil, D.; et al. (2012). "Statistical study of OB stars in NGC 6334 and NGC 6357". Astronomy & Astrophysics. 538: A142. Bibcode:2012A&A...538A.142R. doi:10.1051/0004-6361/201117299.
- ^ "NGC 6334, Cat's Paw Nebula(true color)". earthandskyimaging.com. Earth and sky imaging. October 2019.
- ^ "The Cat's Paw and Lobster Nebulae". www.eso.org. Retrieved 6 February 2017.
- ^ "Protostar blazes and reshapes its stellar nursery". www.eso.org. Retrieved 20 March 2017.
External links
edit- On the Trail of a Cosmic Cat — ESO Photo Release
- NGC 6334 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- Astronomy Picture of the Day - Wide Angle: The Cat's Paw Nebula 2010 April 21
- Cat's Paw Nebula at Constellation Guide