We complement the <scp>parsec</scp> data base of stellar evolutionary tracks with new models of massive stars, from the pre-main-sequence phase to the central carbon ignition. We consider a broad range of metallicities, 0.0001 ≤ <it>Z</it> ≤ 0.04 and initial masses up to <...
Research Assistant
AI chat, annotations, notes & similar papers
No comments yet
Be the first to share your thoughts!