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Trumpler 27

Coordinates:Sky map17h 36m 20s, −33° 31′ 00″
From Wikipedia, the free encyclopedia
Ngc 991
Trumpler 27
Observation data (J2000epoch)
Right ascension17h 36m 20s[1]
Declination−33° 31.0′[1]
Apparent magnitude (V)6.7[1]
Apparent dimensions (V)6 × 6[1]
Physical characteristics
True nature is unknown[2]
Other designationsC 1732-334[1]
Associations
ConstellationScorpius
See also:Open cluster,List of open clusters

Trumpler 27 is a possibleopen cluster in the southern constellationScorpius. If it exists, it is a few thousand light-years away from the Sun, with estimates ranging from 3,900 light-years (1,210 kiloparsecs)[3] to 6,800 light-years (2,100 kiloparsecs)[4] The name refers toRobert Julius Trumpler's catalog of open clusters, published in 1930.[5]

It was originally thought to be young open cluster in the outer edge of theSagittarius Arm, still surrounded byinterstellar matter.[5] The light from the stars is heavilyextinguished andreddened by intervening interstellar dust.[4] The light coming from the stars is also significantly polarized.[6] However, a close study in 2012 could not confirm whether the stars truly form a cluster, or if they are a close alignment of bright stars.[2]

Several member stars have been studied in closer detail. Star #1 of Trumpler 27 isCD−33°12241, ared supergiant star with aspectral type of M0Ia. Stars #28 and #105 areWolf-Rayet stars.[4][7] Star #27, ablue giant star with a spectral type of O8III((f)), may be one of themost luminous stars known, with abolometric magnitude of −10.5.[7] Star #102 is known as V925 Scorpii or HD 159378,[8] and is a rareyellow supergiant star.[9]

See also

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References

[edit]
  1. ^abcde"Cl Trumpler 27".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-03-31.
  2. ^abPerren, G.; Vázquez, R. A.; Carraro, G. (2012). "Photometric distances to young stars in the inner Galactic disk. II. The region towards the open cluster Trumpler 27 at L = 355°".Astronomy and Astrophysics.548: A125.arXiv:1209.3273.Bibcode:2012A&A...548A.125P.doi:10.1051/0004-6361/201219653.S2CID 62888409.
  3. ^Morales, Esteban F. E.; Wyrowski, Friedrich; Schuller, Frederic; Menten, Karl M. (2013). "Stellar clusters in the inner Galaxy and their correlation with cold dust emission".Astronomy and Astrophysics.560: A76.arXiv:1310.2612.Bibcode:2013A&A...560A..76M.doi:10.1051/0004-6361/201321626.S2CID 118422539.
  4. ^abcMoffat, A. F. J.; Fitzgerald, M. P.; Jackson, P. D. (1977). "Trumpler 27: A heavily reddened young open cluster with blue and red supergiants".The Astrophysical Journal.215: 106.Bibcode:1977ApJ...215..106M.doi:10.1086/155338.
  5. ^abThe, P. S.; Stokes, N. (1970). "A study of the southern open clusters : TR 27, TR 28, NGC 6416, NGC 6425".Astronomy and Astrophysics.5: 298.Bibcode:1970A&A.....5..298T.
  6. ^Feinstein, Carlos; Baume, Gustavo; Vazquez, Ruben; Niemela, Virpi; Cerruti, Miguel Angel (2000). "The Highly Polarized Open Cluster Trumpler 27".The Astronomical Journal.120 (4): 1906.arXiv:astro-ph/0007093.Bibcode:2000AJ....120.1906F.doi:10.1086/301562.S2CID 18701893.
  7. ^abMassey, P.;Degioia-Eastwood, K.; Waterhouse, E. (2001). "The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turnoffs. II. Results from 12 Galactic Clusters and OB Associations".The Astronomical Journal.121 (2):1050–1070.arXiv:astro-ph/0010654.Bibcode:2001AJ....121.1050M.doi:10.1086/318769.S2CID 53345173.
  8. ^"HD 159378".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-03-31.
  9. ^Bakker, R.; The, P. S. (1983). "An investigation of the heavily reddened young open cluster TR 27 on the Walraven photometric system".Astronomy and Astrophysics Supplement Series.52: 27.Bibcode:1983A&AS...52...27B.
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