Orion OB1 Association

Orion OB1 Association

The Orion OB1 stellar association is the group of hot giant stars in a large cluster. They are spectral types O and B. There are thousands of lower-mass stars also in this group, and some protostars.

The association is part of the larger Orion Molecular Cloud Complex. It is the most closely studied OB association.

The Orion OB1 association has these subgroups:

Signs of stellar debris disk have been found in the 1a and 1b subgroups. That is a circumstellar disk of dust and debris in orbit around a star.        

References

  1. 1 2 Brown A.G.A.; de Geus E.J.; de Zeeuw P.T. (1994). "The Orion OB1 association. 1: Stellar content". Astronomy and Astrophysics. 289 (1): 101–120. arXiv:astro-ph/9403051. Bibcode:1994A&A...289..101B. ISSN 0004-6361.
  2. ↑ Blaauw, Adriaan (1964). "The O Associations in the Solar neighborhood". Annual Review of Astronomy and Astrophysics. 2 (1): 213–246. Bibcode:1964ARA&A...2..213B. doi:10.1146/annurev.aa.02.090164.001241.
  3. ↑ Briceño, César; Hartmann, Lee; Hernández, Jesús; Calvet; et al. (2007). "25 Orionis: A kinematically distinct 10 mya-old group in Orion OB1a". The Astronomical Journal. 661 (2): 1119–1128. arXiv:astro-ph/0701710. Bibcode:2007ApJ...661.1119B. doi:10.1086/513087. S2CID 118950935.
  4. ↑ Harper, Graham M.; Brown, Alexander; Guinan, Edward F. (2008). "A New VLA-Hipparcos distance to Betelgeuse and its implications". The Astronomical Journal. 135 (4): 1430–40. Bibcode:2008AJ....135.1430H. doi:10.1088/0004-6256/135/4/1430.
  5. ↑ Warren W.H., Jr.; Hesser J.E. (1977). "A photometric study of the Orion OB 1 association. I - Observational data". Astrophysical Journal Supplement Series. 34: 115–206. Bibcode:1977ApJS...34..115W. doi:10.1086/190446.
  6. ↑ Warren W.H., Jr.; Hesser J.E. (1978). "A photometric study of the Orion OB 1 association. III - Subgroup analyses". Astrophysical Journal Supplement Series. 36: 497–572. Bibcode:1978ApJS...36..497W. doi:10.1086/190510.
  7. ↑ N. Calvet et al; The Astronomical Journal 129:935–946 (2005)
  8. ↑ J. Hernandez et al., Astrophys. J. 652:472-481 (2006)