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The Associations OB 110 and OB 112 in M 33 Galaxy
Published online by Cambridge University Press: 04 August 2017
Extract
The associations OB 110 and OB 112 in M 33 galaxy (Humphreys and Sandage, 1980) form a powerful group of young stars. This rich star cloud is situated far (∼6 kpc) from M 33 nucleus. The abundance of hot stars and its huge dimensions (900 × 1500 pc) make it similar to the association OB 78 (400 × 800 pc) in the Andromeda galaxy. We use distance modulus (m-M)v = 25.35 given by Sandage and Carlson (1983) and EB-V = 0.03.
- Type
- Poster Papers 3
- Information
- Symposium - International Astronomical Union , Volume 116: Luminous Stars and Associations in Galaxies , 1986 , pp. 391 - 392
- Copyright
- Copyright © Reidel 1986
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