Serpens south

Serpens South

A cluster of new stars called Serpens South.
Courtesy of NASA/ESA
Observation data (J2000.0 epoch)
Constellation Serpens
Right ascension 18h 30m 03.0s
Declination −2° 01′ 58″
Distance 1420±30 ly[1] (436±9 pc)
Apparent magnitude (V) n/a
Apparent dimensions (V) 14.4×20.3 arcmins
Physical characteristics
Radius 3.5×5 ly

The Serpens South star cluster is a relatively dense group of 50 young stars, 35 of which are protostars just beginning to form. 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.

The cluster was uncovered by NASA's Spitzer Space Telescope. This discovery was made possible by the infrared capabilities of SST, which was necessary because the stars are completely obscured by interstellar dust in the Serpens cloud at visible wavelengths. X-ray observations have also provided detailed information about the stellar cluster.[2] And, the region has served as a laboratory for radio-wavelength studies of star formation in dense molecular filaments.[3]

The discovery of Serpens South is a direct result of the Gould's Belt Legacy project at the Harvard-Smithsonian Center for Astrophysics, which aims to study all prominent star-forming regions within about 1,600 light-years of Earth.[4][5] 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.[1]

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

See also

References

  1. 1 2 Ortiz-León, G. N.; et al. (2016). "The Gould's Belt Distances Survey (GOBELINS) III. The distance to the Serpens/Aquila Molecular Complex". Astrophysical Journal. arXiv:1610.03128Freely accessible. Bibcode:2016arXiv161003128O.
  2. ↑ Winston, E. (2009). "A Chandra Snapshot of Serpens South". Chandra proposal. Bibcode:2009cxo..prop.2775W.
  3. ↑ Kirk, H.; et al. (2013). "Filamentary Accretion Flows in the Embedded Serpens South Protocluster". Astrophysical Journal. 766 (2): 115. arXiv:1301.6792Freely accessible. Bibcode:2013ApJ...766..115K. doi:10.1088/0004-637X/766/2/115.
  4. ↑ Two Telescopes Combine to Probe Young 'Family' of Stars
  5. ↑ Mission statement - Gould's Belt Survey

Coordinates: 18h 30m 03.0s, −02° 01′ 58″

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