A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is application/pdf.
How May Seismological Measurements Constrain Parameters of Stellar Structure?
1993
International Astronomical Union Colloquium
Preserved Fulltext
AbstractPulsation frequency separations, combined with other observations, can constrain the structural parameters of Sun-like stars. As an example, we treat a hypothetical visual binary system resemblingαCen.
doi:10.1017/s025292110001842x
fatcat:kvkt5y3ma5fjxnns3pwessxbj4