Abstract
Evolutionary tracks for a 30 M⊙ star with mass loss rates (0.0, 1.0, 2.5, 5.0, 10.0)x10−7 M⊙/yr have been calculated. The effect of the different rates on the main sequence lifetime and on the effective temperature of the core He burning is discussed.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1979 International Astronomical Union
About this chapter
Cite this chapter
Falk, H.J., Mitalas, R. (1979). Evolution of a 30 M⊙ Star with Mass Loss. In: Conti, P.S., De Loore, C.W.H. (eds) Mass Loss and Evolution of O-Type Stars. International Astronomical Union/Union Astronomique Internationale, vol 83. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-9452-2_53
Download citation
DOI: https://doi.org/10.1007/978-94-009-9452-2_53
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-0989-9
Online ISBN: 978-94-009-9452-2
eBook Packages: Springer Book Archive