We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.
Istituto di Astrofisica e Planetologia Spaziale - INAF email: [email protected]
Marco Limongi
Affiliation:
Osservatorio Astronomico di Roma - INAF email: [email protected]Kavli Institute for the Physics and Mathematics of the Universe, Todai Institutes for Advanced Study, The University of Tokyo, Kashiwa 277-8583, JapanEuropean Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei Munchen, Germany
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
I will briefly review the dependence of the explosive yields on the initial mass, metallicity and initial rotational velocity.