SPECTROSCOPIC NON-ADIABATIC DIAGRAMS FOR MULTIMODAL PULSATING STARS
Recently we proposed a new method of mode identification based on spectroscopic nonadiabatic diagrams (Cugier & Daszynska 2001, As.Ap., 377, 113). Our results are for β Cephei models. These diagram involve the amplitude ratios and phase differences calculated from various oscillating parameters...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Odessa I. I. Mechnykov National University
2017-04-01
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| Series: | Odessa Astronomical Publications |
| Online Access: | http://oap.onu.edu.ua/article/view/99150 |