Table 1: Value of the orbital frequencies at the parametric resonance for the first three modes m and with n=1,2, in the case of a Newtonian gravitational potential. The results are given for a $1.4~M_\odot$ neutron star rotating respectively at 300 and 600 Hz. The value on the left of the symbol/corresponds to the absolute value sign taken to be - and on the right to be +.
Mode m Orbital frequency $\nu(r,a_*)$ (Hz)

$\nu_*=600$ Hz $\nu_*=300$ Hz

n=1 n=2 n=1 n=2

1 -600 / 200 -- / 300 -300 / 100 -- / 150

2 -- / 300 1200 / 400 -- / 150 600 / 200

3 1800 / 360 900 / 450 900 / 180 450 / 225

**Table 1:** Value of the orbital frequencies at the parametric resonance for the first three modes m and with n=1,2, in the case of a Newtonian gravitational potential. The results are given for a $1.4~M_\odot$ neutron star rotating respectively at 300 and 600 Hz. The value on the left of the symbol/corresponds to the absolute value sign taken to be - and on the right to be +.
Mode m	Orbital frequency $\nu(r,a_*)$ (Hz)
	$\nu_*=600$ Hz	$\nu_*=300$ Hz
	n=1	n=2	n=1	n=2
1	-600 / 200	-- / 300	-300 / 100	-- / 150
2	-- / 300	1200 / 400	-- / 150	600 / 200
3	1800 / 360	900 / 450	900 / 180	450 / 225

Source LaTeX | All tables | In the text

	1 Introduction
	2 The model
	3 Results
	4 Conclusion
	References