Results 81 to 90 of about 127 (114)
Measuring cosmological parameters. [PDF]
Freedman WL.
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Galaxies and large scale structure at high redshifts. [PDF]
Steidel CC.
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Subdwarf B Stars: Tracers Of Binary Evolution
Subdwarf B stars are a superb stellar population to study binary evolution. In 2001, Maxted et al. (MNRAS, 326, 1391) found that 21 out of the 36 subdwarf B stars they studied were in short period binaries. These observations inspired new theoretical work that suggests that up to 90 per cent of subdwarf B stars are in binary systems with the remaining ...
Morales-Rueda, L. +2 more
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The abundances of carbon and nitrogen in the atmospheres of classical Be stars. [PDF]
Peters GJ +4 more
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Forty-Four New White Dwarfs in the Southern Hemisphere. [PDF]
Luyten WJ.
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Backtracking the evolution of subdwarf B stars with asteroseismology
Promotor : Aerts, C.C. Co-promotor : Nelemans, G.A.
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A Faint Progenitor System for the Faint Supernova 2024vjm
Zimmerman E +69 more
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The evolution of helium-rich subdwarf-B stars
Astrophysics and Space Science, 2004Helium-rich subdwarf-B (He-sdB) stars are extremely rare hot subluminous stars found in the field of our Galaxy as well as in some globular clusters. The existence of these hot helium stars cannot be explained by canonical stellar evolution theories nor can it be explained by normal sdB evolution.
A. Ahmad, C.S. Jeffery
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