The evolution of massive stars and their spectra - I. A non-rotating 60 M⊙ star from the zero-age main sequence to the pre-supernova stage

@inproceedings{Groh2014TheEO,
  title={The evolution of massive stars and their spectra - I. A non-rotating 60 M⊙ star from the zero-age main sequence to the pre-supernova stage},
  author={Jose H Groh and Georges Meynet and Sylvia Ekstrom and Cyril Georgy},
  year={2014}
}
  • Jose H Groh, Georges Meynet, +1 author Cyril Georgy
  • Published 2014
  • Physics
  • For the first time, the interior and spectroscopic evolution of a massive star is analyzed from the zero-age main sequence (ZAMS) to the pre-supernova (SN) stage. For this purpose, we combined stellar evolution models using the Geneva code and atmospheric models using CMFGEN. With our approach, we were able to produce observables, such as a synthetic high-resolution spectrum and photometry, aiding the comparison between evolution models and observed data. Here we analyze the evolution of a non… CONTINUE READING

    Create an AI-powered research feed to stay up to date with new papers like this posted to ArXiv

    Citations

    Publications citing this paper.
    SHOWING 1-2 OF 2 CITATIONS

    Predicting the nature of supernova progenitors

    • Jose H Groh
    • Physics, Medicine
    • Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
    • 2017
    VIEW 1 EXCERPT
    CITES BACKGROUND

    References

    Publications referenced by this paper.
    SHOWING 1-2 OF 2 REFERENCES

    Physics, Formation and Evolution of Rotating Stars

    VIEW 3 EXCERPTS
    HIGHLY INFLUENTIAL

    Evolution of massive stars and their spectra

    • Groh
    • 1994
    VIEW 3 EXCERPTS
    HIGHLY INFLUENTIAL