Studies in Stellar Structure and Evolution

恒星建模计算将在某些类别恒星生命周期的不同阶段进行。这些都是观察得很好的案例，但还没有建立模型，也没有令人满意的解释。它们包括低质量渐近巨型分支星，9到11个太阳质量的恒星，恒星演化后期的白矮星，共生变星，突变变星，以及紧密白矮星-氦双星中的质量传递。＊＊＊

Iben 9417156 Stellar modeling calculations will be performed on a variety of phases in the lifetimes of certain classes of stars. These are well-observed cases which have not yet been modeled nor explained satisfactorily. They include low-mass asymptotic giant branch stars, stars with 9 to 11 solar masses, white dwarfs in the late stages of stellar evolution, symbiotic variable stars, cataclysmic variable stars, and mass transfer in close white dwarf-helium star binaries. ***