All Tables

Table 1: New $\beta$ Cephei stars. N is the number of independent modes found in the ASAS-3 photometry, the remaining columns are self-explanatory. References to the MK spectral types in the eighth column are the following: (1) Houk & Cowley (1975); (2) Houk (1978); (3) Houk (1982); (4) Houk & Smith-Moore (1988); (5) Houk & Swift (1999); (6) Hill (1970).
Table 3: Possible rotational splittings for seven stars from our sample. Designation of frequencies is the same as in Table 2.
Table 4: Stars with periods longer than 0.4 d.
Table 5: Time of maximum light for both modes detected in HD 168050.
Table 6: Data for the four new $\beta$ Cephei stars in eclipsing systems.
Table 7: The results of the verification of variability of 22 O and early B-type candidate short-period variables observed by Hipparcos and found by Koen (2001) and Koen & Eyer (2002). DT is the detection threshold in the ASAS-3 photometry.
Table 2: Parameters of the sine-curve fits to the V magnitudes of new $\beta$ Cephei-type stars listed in Table 1. $N_{\rm obs}$ is the number of observations, the initial epoch T₀ is equal to 2 450 000.0. The other parameters are the following: $T_{\rm max}^i$ , time of maximum light for the ith mode, $\sigma _{\rm res}$ , standard deviation of the residuals, DT, detection threshold.