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The mass of the white dwarf in the old nova BT Mon

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Figure

Table 1. Times of mid-eclipse for BT Mon.
Figure 1. The average spectrum of BT Mon, uncorrected for orbital motion.
Figure 2. Continuum and emission line light curves of BT Mon. The open circles represent points where the real data, the closed circles, have been folded over.
Figure 3. Orbital emission line variations in BT Mon. The data have been averaged into 10 binary phase bins with a multiple of 2.8 added to each spectrum inorder to displace the data in the y-direction.
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