Stellar progenitors of black holes: Insights from optical and infrared observations

Here are reviewed the insights from observations at optical and infrared wavelengths for low mass limits above which stars do not seem to end as luminous supernovae. These insights are: (1) the absence in archived images of nearby galaxies of stellar progenitors of core-collapse supernovae above 16-...

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Autor principal: Mirabel, I.F.
Formato: SER
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17439213_v12_nS324_p27_Mirabel
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spelling todo:paper_17439213_v12_nS324_p27_Mirabel2023-10-03T16:31:24Z Stellar progenitors of black holes: Insights from optical and infrared observations Mirabel, I.F. black hole physics gravitational waves supernovae: general X-rays: binaries Here are reviewed the insights from observations at optical and infrared wavelengths for low mass limits above which stars do not seem to end as luminous supernovae. These insights are: (1) the absence in archived images of nearby galaxies of stellar progenitors of core-collapse supernovae above 16-18 M⊙, (2) the identification of luminous-massive stars that quietly disappear without optically bright supernovae, (3) the absence in the nebular spectra of supernovae of type II-P of the nucleosynthetic products expected from progenitors above 20 M⊙, (4) the absence in color magnitude diagrams of stars in the environment of historic core-collapse supernovae of stars with ≥20 M⊙. From the results in these different areas of observational astrophysics, and the recently confirmed dependence of black hole formation on metallicity and redshift of progenitors, it is concluded that a large fraction of massive stellar binaries in the universe end as binary black holes. © International Astronomical Union 2017. SER info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_17439213_v12_nS324_p27_Mirabel
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic black hole physics
gravitational waves
supernovae: general
X-rays: binaries
spellingShingle black hole physics
gravitational waves
supernovae: general
X-rays: binaries
Mirabel, I.F.
Stellar progenitors of black holes: Insights from optical and infrared observations
topic_facet black hole physics
gravitational waves
supernovae: general
X-rays: binaries
description Here are reviewed the insights from observations at optical and infrared wavelengths for low mass limits above which stars do not seem to end as luminous supernovae. These insights are: (1) the absence in archived images of nearby galaxies of stellar progenitors of core-collapse supernovae above 16-18 M⊙, (2) the identification of luminous-massive stars that quietly disappear without optically bright supernovae, (3) the absence in the nebular spectra of supernovae of type II-P of the nucleosynthetic products expected from progenitors above 20 M⊙, (4) the absence in color magnitude diagrams of stars in the environment of historic core-collapse supernovae of stars with ≥20 M⊙. From the results in these different areas of observational astrophysics, and the recently confirmed dependence of black hole formation on metallicity and redshift of progenitors, it is concluded that a large fraction of massive stellar binaries in the universe end as binary black holes. © International Astronomical Union 2017.
format SER
author Mirabel, I.F.
author_facet Mirabel, I.F.
author_sort Mirabel, I.F.
title Stellar progenitors of black holes: Insights from optical and infrared observations
title_short Stellar progenitors of black holes: Insights from optical and infrared observations
title_full Stellar progenitors of black holes: Insights from optical and infrared observations
title_fullStr Stellar progenitors of black holes: Insights from optical and infrared observations
title_full_unstemmed Stellar progenitors of black holes: Insights from optical and infrared observations
title_sort stellar progenitors of black holes: insights from optical and infrared observations
url http://hdl.handle.net/20.500.12110/paper_17439213_v12_nS324_p27_Mirabel
work_keys_str_mv AT mirabelif stellarprogenitorsofblackholesinsightsfromopticalandinfraredobservations
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