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Advances in Helio- and Asteroseismology - Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7-11, 1986 (Paperback, Softcover reprint of the original 1st ed. 1988)
Loot Price: R1,712
Discovery Miles 17 120
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Advances in Helio- and Asteroseismology - Proceedings of the 123th Symposium of the International Astronomical Union, Held in Aarhus, Denmark, July 7-11, 1986 (Paperback, Softcover reprint of the original 1st ed. 1988)
Series: International Astronomical Union Symposia, 123
Expected to ship within 10 - 15 working days
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Helio- and asteroseismology study the interior of the Sun and other
stars, by means of observations of oscillations on their surfaces.
The last 10 years in the study of the solar interior, to a has
witnessed a very rapid evolution point where we can now contemplate
investigating the physical state of matter, or the details of
rotation and other large-scale motion, in the Sun. The stellar
studies are in some respects at the point of the solar studies 10
years ago, but appear poised to take off. Thus the time was deemed
ripe for lAO Symposium No 123, to assess the present status of this
work, and plan for its future development. Apart from the seismic
data, few observations are available to provide information about
stellar interiors. Detailed studies, by spectral analysis, can be
made of stellar surface properties, including atmospheric
temperature and chemical composition. However, the stellar
radiative spectrum is almost entirely fixed by the mass,
luminosity, radius and surface rotation of the star, and contains
essentially no other information about the interior. An important
test of stellar evolution theory is provided by observations of
stel lar clusters, whose members can reasonably be assumed to have
the same age and chemical composition. The location of such stars
in a HR diagram, where luminosity is plotted against the effective
temperature, can roughly be understood in terms of stellar
evolution calculations."
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