Serpens South Explained

Serpens South
Type:Emission
Epoch:J2000.0
Ra:[1]
Dist Ly:1422 ± 30 ly
Dist Pc:[2]
Size V:14.4 × 20.3 arcmins
Constellation:Serpens
Radius Ly:3.5 × 5 ly

The Serpens South star cluster is a relatively dense group of more than 600 young stars, dozens of which are protostars just beginning to form.[3] The cluster is situated in the southern portion of the Serpens cloud (adjacent to the star-forming region known as W40). The stars are embedded in a dense filament of interstellar gas, which is part of the giant molecular cloud that has given rise to the cluster of young stars in W40. This entire complex is located at a distance of 1420 light-years (436 pc) from the Earth, and is approximately the same distance as the Serpens Main cluster.[2]

The cluster was uncovered by NASA's Spitzer Space Telescope.[4] This discovery was made possible by the infrared capabilities of this space telescope, which were necessary because the stars are completely obscured by interstellar dust in the Serpens cloud at visible wavelengths. Hundreds of young stellar objects have been detected at mid-infrared objects using these data.[5] X-ray observations by NASA's Chandra X-ray Observatory have also provided detailed information about the stellar cluster.[6] [7] And, the region has served as a laboratory for radio-wavelength studies of star formation in dense molecular filaments.[8]

The discovery of Serpens South is a direct result of the Gould's Belt Legacy project at the Center for Astrophysics Harvard & Smithsonian, which aims to study all prominent star-forming regions within about 1,600 light-years of Earth.[9] [10] The Gould Belt is a ring of molecular clouds and associated star-forming regions first described by astronomer Benjamin Gould in 1879. Although the Serpens Molecular cloud is too distant to formally be considered a member of the Gould Belt, it is often included in Gould Belt surveys.

Serpens South is located half a degree west of the main W40 cluster and three degrees south of the Serpens Main cluster.

See also

External links

Notes and References

  1. NAME Serpens South Cluster. 11 April 2018.
  2. Ortiz-León . G. N. . etal . 2016 . The Gould's Belt Distances Survey (GOBELINS) III. The distance to the Serpens/Aquila Molecular Complex . The Astrophysical Journal . 834 . 2 . 143 . 1610.03128 . 10.3847/1538-4357/834/2/143 . 2017ApJ...834..143O . 10802135 . free .
  3. Maury. A. J.. André. P.. Men'shchikov. A.. Könyves. V.. Bontemps. S.. The formation of active protoclusters in the Aquila rift: a millimeter continuum view. Astronomy & Astrophysics. 535. 2011. A77. 0004-6361. 10.1051/0004-6361/201117132. 2011A&A...535A..77M. 1108.0668 . 119285813 .
  4. Gutermuth. R. A.. Bourke. T. L.. Allen. L. E.. Lori Allen (astronomer). Myers. P. C.. Megeath. S. T.. Matthews. B. C.. Jørgensen. J. K.. Di Francesco. J.. Ward-Thompson. D.. Huard. T. L.. Brooke. T. Y.. Dunham. M. M.. Cieza. L. A.. Harvey. P. M.. Chapman. N. L.. TheSpitzerGould Belt Survey of Large Nearby Interstellar Clouds: Discovery of a Dense Embedded Cluster in the Serpens-Aquila Rift. The Astrophysical Journal. 673. 2. 2008. L151–L154. 0004-637X. 10.1086/528710. 2008ApJ...673L.151G. 0712.3303 . 339753 .
  5. Povich. Matthew S.. Kuhn. Michael A.. Getman. Konstantin V.. Busk. Heather A.. Feigelson. Eric D.. Broos. Patrick S.. Townsley. Leisa K.. King. Robert R.. Naylor. Tim. THE MYStIX INFRARED-EXCESS SOURCE CATALOG. The Astrophysical Journal Supplement Series. 209. 2. 2013. 31. 0067-0049. 10.1088/0067-0049/209/2/31. 1309.4497 . 2013ApJS..209...31P . 62807763 .
  6. Winston . E. . 2009 . A Chandra Snapshot of Serpens South . Chandra Proposal . 11200492. 2009cxo..prop.2775W.
  7. Getman . etal . 2016 . Star Formation In Nearby Clouds (SFiNCs): X-ray And Infrared Source Catalogs And Membership . 1612.05282 . 10.3847/1538-4365/229/2/28 . 229 . The Astrophysical Journal Supplement Series . 2 . 28. 2017ApJS..229...28G . 59124520 . free .
  8. Kirk . H. . etal . 2013 . Filamentary Accretion Flows in the Embedded Serpens South Protocluster . Astrophysical Journal . 766 . 2 . 115 . 10.1088/0004-637X/766/2/115 . 2013ApJ...766..115K . 1301.6792 . 55835836 .
  9. http://www.physorg.com/news105801659.html Two Telescopes Combine to Probe Young 'Family' of Stars
  10. http://www.cfa.harvard.edu/gouldbelt/ Mission statement - Gould's Belt Survey

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