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The Explosion of Helium Stars Evolved with Mass Loss

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This article is published in The Astrophysical Journal.The article was published on 2020-02-12 and is currently open access. It has received 134 citations till now. The article focuses on the topics: Stars & Helium.

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Stripped-envelope stars in different metallicity environments. II. Type I supernovae and compact remnants

TL;DR: In this article , the authors use grids of core-collapse models obtained from helium stars at different metallicities to study the effects of metallicity on the transients and remnants these stars produce.
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Constraints on the Explosion Timescale of Core-collapse Supernovae Based on Systematic Analysis of Light Curves

TL;DR: In this paper , the authors analyzed multiband light curves of 82 stripped-envelope supernovae (SESNe) to obtain bolometric light curves, which are among the largest samples of the bolometre light curves derived from the multiband spectral energy distribution.
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Stars Stripped in Binaries: The Living Gravitational-wave Sources

TL;DR: In this article, the authors developed a Monte Carlo code that uses detailed evolutionary models to simulate the Galactic population of stripped stars in tight orbits with either neutron star or white dwarf companions, and showed that stripped star binaries are promising multi-messenger sources for the upcoming electromagnetic and gravitational wave facilities.
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On the Neutron Star/Black Hole Mass Gap and Black Hole Searches

TL;DR: In this paper , the authors collected the compact objects that are probable black holes with masses being in the gap, and described the theoretical predictions for the formation of black holes in various types of binaries, and present some prospects of searching for black holes via electromagnetic and gravitational wave observations.
References
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Journal ArticleDOI

The Luminosity function and stellar evolution

TL;DR: In this paper, the evolutionary significance of the observed luminosity function for main-sequence stars in the solar neighborhood is discussed and it is shown that stars move off the main sequence after burning about 10 per cent of their hydrogen mass and that stars have been created at a uniform rate in a solar neighborhood for the last five billion years.
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Solar System Abundances and Condensation Temperatures of the Elements

TL;DR: In this article, solar photospheric and meteoritic CI chondrite abundance determinations for all elements are summarized and the best currently available photosphere abundances are selected, including the meteoritic and solar abundances of a few elements (e.g., noble gases, beryllium, boron, phosphorous, sulfur).
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The evolution and explosion of massive stars

TL;DR: In this article, the authors examined the current understanding of the lives and deaths of massive stars, with special attention to the relevant nuclear and stellar physics, and focused on their post-helium-burning evolution.
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Binary Interaction Dominates the Evolution of Massive Stars

TL;DR: More than 70% of all massive stars will exchange mass with a companion, leading to a binary merger in one-third of the cases, greatly exceed previous estimates and imply that binary interaction dominates the evolution of massive stars, with implications for populations ofmassive stars and their supernovae.
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