作者: R.W. Hilditch , S.E. de Mink , O.R. Pols
DOI: 10.1051/0004-6361:20067007
关键词: Stellar mass 、 Astrophysics 、 Binary star 、 Astronomy 、 Small Magellanic Cloud 、 Stellar evolution 、 Metallicity 、 Primary (astronomy) 、 Binary number 、 Physics 、 Mass transfer
摘要: … for the mass transfer efficiency. We address the problem of mass transfer efficiency by fitting … the combination of a large primary mass with a relatively low temperature which cannot be …