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pro vyhledávání: '"Johnathan Hodge"'
Autor:
Tomomi Otani, Andrzej Baran, Ted von Hippel, Brian Herbster, Lorena Sanabria, Johnathan Hodge
Subdwarf B (sdB) stars are post-main-sequence stars of high temperature (22,000 to 40,000 K) and gravity (log g = 5.0 to 6.2). Their formation and evolution are still not well understood but the most promising formation he most promising formation sc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::02cef4e16a85bbe65b4674936f489db4
