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1995 (EN)
Erratum: Axial modes for relativistic stars

Kokkotas, Konstantinos

The paper `Axial modes for relativistic stars' was published in Mon. Not. R. Astron. Soc. 268, 1015-1018 (1994). In this paper there is a systematic numerical error in the numerical calculation which changes the quantitative behaviour of the imaginary part of the axial mode frequencies, but the qualitative picture is exactly the same. The origin of the error can be traced back to the original paper by Chandrasekhar & Ferrari (1991), mainly in their equation (19) which has various misprints. The correct versions of Tables 1 and 2 are reproduced here

Article / Άρθρο
info:eu-repo/semantics/article

Gravitation
Neutron stars
Radiation mechanisms non thermal
Stellar oscillations

Αριστοτέλειο Πανεπιστήμιο Θεσσαλονίκης (EL)
Aristotle University of Thessaloniki (EN)

English

1995
2009-06-29T16:58:45Z


Αριστοτέλειο Πανεπιστήμιο Θεσσαλονίκης, Σχολή Θετικών Επιστημών, Τμήμα Φυσικής

Monthly Notices of the Royal Astronomical Society, vol.277 no.4 [1995] pp. 1599-1599 [Published Version]

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