2 papers
astro-ph1997
On the Velocity and Intensity Line Asymmetries
M. Gabriel
We show that, if solar 5 min. oscillations are excited by convection in the upper layers of the convective envelope, it is impossible to explain the opposite line asymmetries obser…
astro-ph1997
Influence of heavy element and rotationally induced diffusions on the solar models
M. Gabriel
We present the results of solar model computation done with the latest Livermore opacities. Models without diffusion, with hydrogen diffusion only and with hydrogen and heavy eleme…