Mode and period changes in pulsating stars near the main sequence: δ Scuti stars-Reference-Cited by-同舟云学术

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Mode and period changes in pulsating stars near the main sequence: δ Scuti stars

Published:1999-09 Issue:6-7 Volume:43 Page:441-447
ISSN:1387-6473
Container-title:New Astronomy Reviews
language:en
Short-container-title:New Astronomy Reviews

Author:

Breger M.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference32 articles.

1. Alexander, D.R. & Ferguson, J.W., 1994, ApJ, 437, 879.

2. Arellano Ferro, A., Nuñez, N.S., & Avila, J.J., 1994, PASP, 106, 696.

3. Breger, M., 1980, ApJ, 235, 153.

4. Breger, M., 1990, ASPC, 11, 263.

5. Breger, M. & Pamyatnykh, A.A., 1998, A&A, in press.

Cited by 4 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Behaviour of the periods in double mode RR Lyrae, V26 in M15;Astronomy & Astrophysics;2002-08

2. Testing the bivariate series of Mira light curve rise and fall times for changes;Monthly Notices of the Royal Astronomical Society;2001-08-11

3. Stability of pulsation of the double-mode high-amplitudeδScuti star AE Ursae Majoris;Astronomy & Astrophysics;2001-03

4. A revised catalogue of δ Sct stars;Astronomy and Astrophysics Supplement Series;2000-06

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