| Issue |
A&A
Volume 586, February 2016
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 1 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/201526593e | |
| Published online | 22 January 2016 | |
Asteroseismic model fitting by comparing ϵnℓ values (Corrigendum)
Astronomy Unit, Queen Mary University of London Mile End Road London E1 4NS UK
e-mail:
I.W.Roxburgh@qmul.ac.uk
Key words: stars: oscillations / asteroseismology / stars: interiors / methods: analytical / methods: numerical / errata, addenda
The caption to Fig. 2 should be
|
Fig. 2
Superposed curves for the outer phase shifts αℓ(ν,t) of Model A at 3 frequencies. The values of αℓ are independent of ℓ until deep inside the star. |
The caption to Fig. 3 should be
|
Fig. 3
Frequency differences: Model G – Model A. |
References
- Roxburgh, I. W. 2016, A&A, 585, A63 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© ESO, 2016
All Figures
|
Fig. 2
Superposed curves for the outer phase shifts αℓ(ν,t) of Model A at 3 frequencies. The values of αℓ are independent of ℓ until deep inside the star. |
|
| In the text | |
|
Fig. 3
Frequency differences: Model G – Model A. |
|
| In the text | |
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