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Table 1.

Key observational data for known γ Cas stars taken from Nazé & Motch (2018, their Table 5).

No. Name Spectral type log(LX/Lbol) LX LX, hard Hardness ratio kT v sin i
1031 erg s−1 1031 erg s−1 keV km s−1
1 γ Cas B0IV-Vpe −5.39 85.0 65.1 3.25 14−25 295
3 V782 Cas B2.5III:[n]e+ −5.25 30.3 29.9 63.1 7
17 PZ Gem(high) O9pe −6.14 9.66 7.87 4.32 16 265
26 HD90563 B2Ve −5.85 32.0
34 BZ Cru B0.5IVpe −5.69 27.6 20.3 2.81 13 338
37 HD119682 B0Ve −5.63 66.7 47.9 2.55 8−17 200
39 V767 Cen B2Ve −5.37 26.2 17.4 1.97 6 100
40 CQ Cir B1Ve −4.30 175 147 5.26 9 335
47 V759 Ara B2Vne −5.29 41.9 31.9 3.21 10 277
51 V3892 Sgr Oe −5.78 30.8 21.2 2.24 7−14 260
53 V771 Sgr B3/5ne −4.64 24.5 21.1 6.29 8
54 HD316568 B2IVpe −6.26 4.04 2.43 1.60 4−6
75 V2156Cyg B1.5nnpe −5.30 7.53 6.51 6.34 3
79 π Aqr B1Ve −5.59 7.44 5.80 3.56 12 243
83 V810 Cas B1npe −5.14 48.4 41.1 5.58 64 422

Notes. Soft and hard X-ray fluxes refer to the 0.5−2.0 keV and 2.0−10.0 keV intervals, respectively.

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