NGC 6334, colloquially known as the Cat's Paw Nebula, Bear Claw 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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![]() Infrared image of the Cat's Paw Nebula. Green areas showing regions where radiation from hot stars collided with large molecules and small dust grains called "polycyclic aromatic hydrocarbons" (PAHs), causing them to fluoresce | |
Observation data: J2000 epoch | |
Right ascension | 17 20 50.9h [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 |
See also: Lists of nebulae |
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]
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See also: Gum Nebula |
New General Catalogue 6000 to 6499 | |
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