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Table 1:

Axion luminosities and axion masses necessary to account for the observed drift of the period of pulsation of G117-B15A.
Model $L_{\rm ax}/ 10^{30}$ (erg/s) $m_{\rm ax} \cos^2\beta$ (meV)
C 0.6 (2.8/0.0) 2.8 (6.0/0.0)
BK (thick) 6.8 (8.7/4.9) 9.3 (10.6/7.9)
BK (thin) 2.2 (3.5/1.0) 5.5 ( 6.9/3.7)

Source LaTeX | All tables | In the text

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