Trumpler 16

Trumpler 16

The inner region of the Carina Nebula as seen in near-infrared. Trumpler 16 is the cluster of stars at the left, around Eta Carinae (the brightest star in the image).
Observation data (J2000 epoch)
Constellation Carina
Right ascension 10h 45m 10s[1]
Declination −59° 43′ 00″[1]
Distance 9,270 ly (2,842 pc)[1]
Apparent magnitude (V) 5.0[1]
Physical characteristics
Other designations C 1043-594, Cl VDBH 105, OCl 829.0, [KPR2004b] 265, [KPS2012] MWSC 1850[1]

Trumpler 16 (Tr 16) is a massive open cluster that is home to some of the most luminous stars in the Milky Way Galaxy. It is situated within the Carina Nebula complex in the Carina–Sagittarius Arm, located approximately 9,270 ly (2,842 pc) from Earth.[1] The cluster has one naked eye member star, Eta Carinae.

Its most luminous members are Eta Carinae and WR 25, with both having luminosities several million times that of the Sun, and there are six other extreme stars with O3 spectral classes.[2] Both Eta Carinae and WR 25 are binaries, with the primary stars contributing most of the luminosity, but with companions which are themselves more massive and luminous than most stars. Across all wavelengths, WR 25 is estimated to be the more luminous of the two, 6,300,000 times the Sun's luminosity (absolute bolometric magnitude -12.25) compared to Eta Carinae at 5,000,000 times the Sun's luminosity (absolute bolometric magnitude -12.0). However, Eta Carinae appears by far the brightest object, both because it is brighter in visual wavelengths and because it is embedded in nebulosity which exaggerates the luminosity. WR 25 is very hot and emits most of its radiation as ultraviolet.

Trumpler 16 and Trumpler 14 are the most prominent star clusters in Carina OB1, a giant stellar association in the Carina spiral arm. Another cluster within Carina OB1, Collinder 228, is thought to be an extension of Trumpler 16 appearing visually separated only because of an intervening dust lane. The spectral types of the stars indicate that Trumpler 16 formed by a single wave of star formation. Because of the extreme luminosity of the stars formed, their stellar winds push away the clouds of dust, similar to the Pleiades. In a few million years, after the brightest stars have exploded as supernovae, the cluster will slowly die away. Trumpler 16 includes most of the stars in the eastern portion of the Carina OB1 association.[3]

References

  1. 1 2 3 4 5 6 "Trumpler 16". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2 December 2016.
  2. ↑ Wolk, Scott J.; Broos, Patrick S.; Getman, Konstantin V.; Feigelson, Eric D.; Preibisch, Thomas; et al. (May 2011). "The Chandra Carina Complex Project View of Trumpler 16". The Astrophysical Journal Supplement. 194 (1). 12. arXiv:1103.1126Freely accessible. Bibcode:2011ApJS..194...12W. doi:10.1088/0067-0049/194/1/12.
  3. ↑ Carraro, G.; Romaniello, M.; Ventura, P.; Patat, F. (May 2004). "The star cluster Collinder 232 in the Carina complex and its relation to Trumpler 14/16". Astronomy and Astrophysics. 418 (2): 525–537. arXiv:astro-ph/0401144Freely accessible. Bibcode:2004A&A...418..525C. doi:10.1051/0004-6361:20034335.

Further reading

Media related to Trumpler 16 at Wikimedia Commons

Coordinates: 10h 45m 10s, −59° 43′ 00″

This article is issued from Wikipedia - version of the 12/4/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.