Kukarkin, B V. Published by IPST (1975)

Kukarkin, B V. Published by IPST (1975). ISBN 10: 0706513428 ISBN 13: 9780706513424.

Part of the Astrophysics and Space Science Library book series (ASSL, volume 351). We describe the basic properties of radial and non-radial oscillations, their effect on the stellar surface and emitted flux, and the consequences for the observer

A slowly pulsating B-type star (SPB), formerly known as a 53 Persei variable, is a type of pulsating variable star

A slowly pulsating B-type star (SPB), formerly known as a 53 Persei variable, is a type of pulsating variable star. They display variability both in their light emission and in their spectral line profile

In Volume 1 we discussed briefly how this can be understood.

In Volume 1 we discussed briefly how this can be understood. They are similar to the eigenfrequencies of a rope of length 2l, which is fastened at both ends but free to oscillate in the center (see Fig. 18. la).

B. V. Kukarkin's scientific contributions.

Used for: Pulsating variables. Quasars and Pulsars (Portland, OR: North Pacific Publishers, 1971), by Dewey B. Larson (HTML at reciprocalsystem. Items below (if any) are from related and broader terms.

Star formation is closely coupled to planet formation, in ways that are still not well understood.

Steward astronomers attack these problems with observations at many wavelengths and with theoretical calculations. Star formation is closely coupled to planet formation, in ways that are still not well understood.

Astrophysics Solar and Stellar Astrophysics. 8 pages, 5 figures, . Authors:Michel Breger. Submitted on 25 Jan 2010). Many of these modulations are nearly periodic. Subjects: Solar and Stellar Astrophysics (astro-ph. 4443v1 for this version).