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Using a simple model of low-mass stellar objects we have shown modified gravity impact on their early evolution, such as Hayashi tracks, radiative core development, effective temperature, masses, and luminosities.… Click to show full abstract
Using a simple model of low-mass stellar objects we have shown modified gravity impact on their early evolution, such as Hayashi tracks, radiative core development, effective temperature, masses, and luminosities. We have also suggested that the upper mass' limit of fully convective stars on the Main Sequence might be different than commonly adopted.
Keywords:
stellar objects;
mass;
modified gravity;
mass stellar;
low mass
Journal Title: Physical Review D
Year Published: 2020
Link to full text (if available)
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Journal Title: Physical Review D
Year Published: 2020
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!