STELLAR WINDS 1 OBSERVATIONAL EVIDENCE FOR A HOT-COOL STAR CONNECTION Wayne L. Waldron Applied ... 2*1^2) to the bolometric luminosity and the terminal velocity (vw) of the stellar wind to the stellar effective temperature. ... and V*^eff ac The surprising result is that all spectral types throughout the HR diagram are represented in these correlations. ... stellar escape speed, while Cassinelli and Abbott (1981 ) and Underhill (1983) found a relation between v^ and Teff .
|Title||:||The Origin of Nonradiative Heating/momentum in Hot Stars|
|Author||:||Anne Barbara Underhill, A. G. Michalitsianos|