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- W4386850093 abstract "The recently discovered Gaia BH1 binary system, a Sun-like star and a dark object (presumably a black hole), may significantly change our understanding of the population of binaries. The paper presents the components mass ratio (q) distributions of binary systems of different observational classes. They all show a significant shortage of low-q systems. In this work, I demonstrate (quantitatively) how our ignorance extends, and point out the importance of discovering and studying systems like Gaia BH1. In addition, an approximate mass–temperature relation and mass ratio–magnitude difference relation for main-sequence stars are presented here." @default.
- W4386850093 created "2023-09-20" @default.
- W4386850093 creator A5072743113 @default.
- W4386850093 date "2023-09-18" @default.
- W4386850093 modified "2023-09-27" @default.
- W4386850093 title "Gaia BH1: A Key for Understanding the Demography of Low-q Binaries in the Milky Way Galaxy" @default.
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- W4386850093 doi "https://doi.org/10.3390/galaxies11050098" @default.
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