Chapter 12 - Pre-supernova evolution of massive stars
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The primary goal is to investigate the previously indeterminate characteristics of the velocity spectra for the ejected component, including possible maxima and ...
16671 - Unveiling the nature of interacting supernovae or supernova ...
The primary goal is to investigate the previously indeterminate characteristics of the velocity spectra for the ejected component, including possible maxima and ...
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Terminal nodes with a majority of signal events are called signal leaves; otherwise they are background leaves. When new events are evaluated using the decision ...
Core-collapse supernovae and the Younger Dryas/terminal ...
Determining a true upper-mass limit will rely on advances in stellar evolutionary modeling, core-collapse supernova theory, and a wealth of.
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We found that the terminal momentum for clustered SNe did not converge until we reached peak resolutions better than 0.1 pc, far higher than the.
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Among gap transients, stellar mergers can release around 1049 erg. Alternatively, some massive stars can also undergo non-terminal eruptions and outbursts (and ...
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However, the hydrogen in these models moves much faster. Figure 10. Light curves and terminal velocities for a supernova derived from a. 20 M ...