Tracked shipping to New Zealand with premium packaging for just NZ$15 

Ship to
New Zealand
0

My Account

  • argentina
  • chile
  • colombia
  • españa
  • méxico
  • perú
  • estados unidos
  • internacional

menu

Select your country

Americas

Europe

Rest of the world

portada advances in helio- and asteroseismology
Type
Physical Book
Illustrated by
Publisher
Author
Year
1987
Language
English
Pages
628
Format
Paperback
Dimensions
25.4x17.8x3.2 cm
Weight
1.08 kg.
ISBN
9027726159
ISBN13
9789027726155
Categories

advances in helio- and asteroseismology

Jørgen Christensen-Dalsgaard (Illustrated by) · Søren Frandsen (Illustrated by) · Springer · Paperback

advances in helio- and asteroseismology - Christensen-Dalsgaard, Jørgen ; Frandsen, Søren

Cheaper New Book Imported to New Zealand
Delivery: 03 Nov - 13 Nov Shipping: 15 to 19 business days.
NZ$ 127.50
Faster New Book Imported to New Zealand
Delivery: 21 Oct - 28 Oct Shipping: 6 to 7 business days.
NZ$ 160.89
Import costs and 15% GST included in the price ✅
NZ$ 127.50

Choose the list to add your product or create one New List

Go to My Wishlists
Calculate shipping cost

Synopsis "advances in helio- and asteroseismology"

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.

Customers reviews

More customer reviews
  • 0% (0)
  • 0% (0)
  • 0% (0)
  • 0% (0)
  • 0% (0)

Frequently Asked Questions about the Book

Is the book original?

All books in our catalog are Original.

In what language is the book written?

The book is written in English.

What is the format of this book?

The binding of this edition is Paperback.

Questions and Answers about the Book

Do you have a question about the book? Login to be able to add your own question.

Opinions about Bookdelivery

More customer reviews