... require membership in a close binary ; for 35M , _ radiative mass loss will suffice ... Two additional models were extracted from a 35M star at carbon ignition. ... case (1.78 M in the 25 M derived _ _ models ; 2.03 M for the 35M derived models ...
... 20/72 Mechanical Luminosity L w 10 34 н 10 35 W § Mass-loss M w 1 M sun y н 1 ... н 3 = 10 13 ergs s н 1 cm 3 that a typical value in SI units is 10 н 35 W m 3 s н 1 ...
... matter at the time dark matter decoupled td m d ec is determined by the fraction of relativistic degrees of freedom that were associated with dark matter at that time (see Eq. 14). with = -1.35 at M < 0.5M and = -2.35+0..65 at M -0 35 0.5M (Elmegreen 2007 ...
... Cartesian tensors 29/35 (42) · If i = m we only get a contribution from the terms s i and k i, s . Consequently k = p . ... ip km Cartesian tensors (43) 30/35 6.5 Application of iks mps [ curl ( u в v ) ] i = ijk ( klm u l v m ) x j = ijk klm ( ul vm ...
... Vol. 560 logical models ) \ 0.35, ) \ 0.65 (favored), ) \ M " M 0.35, ) \ 0.0 (open), ) \ 1.00, ) \ 0.0 (Einsteinхde " M model representing a progres" Sitter), and an astrophysical sive dimming in proportion to redshift caused by gray dust or simple ...