NGC 6357

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NGC 6357 is a diffuse nebula near NGC 6334 in the constellation Scorpius. The nebula contains many proto-stars shielded by dark discs of gas, and young stars wrapped in expanding "cocoons" or expanding gases surrounding these small stars. It is also known as the Lobster Nebula.[1][2] This nebula was given the name War and Peace Nebula by the Midcourse Space Experiment scientists because of its appearance, which, in infrared images the bright, western part resembles a dove, while the eastern part looks like a skull.[3] A petition by anime fans to rename it as the Madokami nebula, due to resemblance with a character, was unsuccessful.[4][5]

It is located about 5,500 light years away from Earth.[6] NGC 6357 is connected by a filamentary structure to NGC 6334, and the two may form a single complex.[7]

Associated open clusters

Pismis 24

File:EmissionNebula NGC6357.jpg
A Hubble Space Telescope (HST) image of Pismis 24-1, the "core" of NGC 6357.
File:NGC 6357.jpg
Dark Energy Camera captures the star-forming nebula NGC 6357

This nebula includes the open cluster Pismis 24, which is home to several massive stars. One of the brightest stars in the cluster, Pismis 24-1, was thought possibly to be the most massive on record, approaching 300 solar masses, until it was discovered to be a multiple system of at least three stars; component stars would still remain near 100 solar masses each, making them among the more massive stars on record.[8][9]

G353.2+0.7

The young stellar cluster G353.2+0.7 lies east of Pismis 24 and was revealed by a Chandra X-ray image showing approximately 800 stars.[10]

G353.1+0.6

The young stellar cluster G353.1+0.6 lies southeast of Pismis 24 and also contains approximately 800 stars detected by X-ray.[10] The region includes several O-type stars, including [BDSB2003] 10.[11]

Massive stars

NGC 6357 is one of the most prominent sites of massive-star formation in our neighborhood of the Milky Way. A variety of early O-type stars reside in this nebula, blowing the bubbles around the star clusters that can be seen in the molecular cloud.

Prominent stars in Pismis 24[12]
Star name Spectral type Magnitude
(Mbol)
Temperature[13]
(K)
Radius
(Template:Solar radius)
Mass
(Template:Solar mass)
WR 93 (HD 157504) WC7 -11.2 71,000 10 120
Pismis 24-1NE O3.5 If* −10.0 42,000 17 74
Pismis 24-1SW O4 III −9.8 41,500 16 66
Pismis 24-2 O5.5 V(f) −8.9 40,000 12 43
Pismis 24-3 O8 V −7.7 33,400 9 25
Pismis 24-10 O9 V −7.2 31,500 8 20
Pismis 24-12 B1 V −5.3 30,000 4 11
Pismis 24-13 O6.5 III((f)) −8.6 35,600 12 35
Pismis 24-15 O8 V −7.8 33,400 10 25
Pismis 24-16 O7.5 V −9.0 34,000 16 38
Pismis 24-17 O3.5 III −10.1 42,700 17 78
Pismis 24-18 B0.5 V −6.4 30,000 6 15
Pismis 24-19 B0.5 V −5.4 30,000 4 11

See also

References

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External links

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  1. Star Forming Region NGC 6357 showing complex interactions between interstellar winds, radiation pressures and magnetic fields.
  2. A Massive Star in NGC 6357 with a close-up of Pismis 24.
  3. NGC 6357: Cathedral to Massive Stars
  4. A Massive Star in NGC 6357
  5. NGC 6357: Cathedral to Massive Stars
  6. NGC 6357: The Lobster Nebula

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