NGC 6357

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NGC 6357
Emission nebula
H II region
Cosmic ‘Winter’ Wonderland.jpg
NGC 6357 composite image
Credit: X-ray: NASA/CXC/PSU/L.Townsley et al.; Optical: UKIRT; Infrared: NASA/JPL-Caltech
Observation data: J2000 epoch
Right ascension 17h 24m[1]
Declination−34° 20′[1]
Distance~5900±450[2] ly   (1800±140 pc)
ConstellationScorpius[3]
DesignationsWar and Peace Nebula,[1] Lobster Nebula [4] Sharpless 11, RCW 131, Gum 66
See also: Lists of nebulae

NGC 6357 is a diffuse nebula near NGC 6334 in the constellation Scorpius. The nebula contains many proto-stars shielded by dark disks of gas, and young stars wrapped in expanding "cocoons" or expanding gases surrounding these small stars. It is also known as the Lobster Nebula.[4][5]

This nebula was also 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.[6]

It is located about 5500 light years away from Earth.[7]

Associated Open Clusters[edit]

Pismis 24[edit]

A Hubble Space Telescope (HST) image of Pismis 24-1, the "core" of 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[edit]

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[edit]

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[edit]

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

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

References[edit]

  1. ^ a b c "NGC 6357". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2007-05-03.
  2. ^ Kuhn, Michael A.; Hillenbrand, Lynne A.; Sills, Alison; Feigelson, Eric D.; Getman, Konstantin V. (2018). "Kinematics in Young Star Clusters and Associations with Gaia DR2". The Astrophysical Journal. 870 (1): 32. arXiv:1807.02115. Bibcode:2019ApJ...870...32K. doi:10.3847/1538-4357/aaef8c.
  3. ^ R. W. Sinnott, ed. (1988). The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer. Sky Publishing Corporation and Cambridge University Press. ISBN 978-0-933346-51-2.
  4. ^ a b Sample, Ian (20 February 2013). "Lobster Nebula – birthplace of stars – revealed in infrared". the Guardian.
  5. ^ "Lobster Nebula Seen with ESO's VISTA Telescope Space Wallpaper".
  6. ^ "2MASS Picture of the Week Archive Captions".
  7. ^ "Winter Wonderland' Glows in Space as Nebula Is Wreathed in Wintry Colors". Space.com.
  8. ^ "ESA Science & Technology: Star on a Hubble diet NGC 6357". Archived from the original on 2007-04-04. Retrieved 2007-04-11.
  9. ^ Nemiroff, R.; Bonnell, J., eds. (19 December 2006). "NASA: Massive Stars in Open Cluster Pismis 24". Astronomy Picture of the Day. NASA.
  10. ^ a b Townsley, L. K.; et al. (2014). "The Massive Star-Forming Regions Omnibus X-Ray Catalog". Astrophysical Journal Supplement. 213 (1): 1. arXiv:1403.2576. Bibcode:2014ApJS..213....1T. doi:10.1088/0067-0049/213/1/1.
  11. ^ Damke, G.; et al. (2006). "The open cluster G353.1+0.7 in NGC6357". Revista Mexicana de Astronomía y Astrofísica. 26: 180. Bibcode:2006RMxAC..26..180D.
  12. ^ Fang, M.; Van Boekel, R.; King, R. R.; Henning, T.; Bouwman, J.; Doi, Y.; Okamoto, Y. K.; Roccatagliata, V.; Sicilia-Aguilar, A. (2012). "Star formation and disk properties in Pismis 24". Astronomy & Astrophysics. 539: A119. arXiv:1201.0833. Bibcode:2012A&A...539A.119F. doi:10.1051/0004-6361/201015914.
  13. ^ Martins, F.; Schaerer, D.; Hillier, D. J. (2005). "A new calibration of stellar parameters of Galactic O stars". Astronomy and Astrophysics. 436 (3): 1049–1065. arXiv:astro-ph/0503346. Bibcode:2005A&A...436.1049M. doi:10.1051/0004-6361:20042386.

External links[edit]

  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