Abstract
We present a detailed, quantitative study of the standard [WC10] Wolf-Rayet central star CPD-56o 8032 based on new high resolution AAT UCLES observations and the Hillier (1990) WR standard model. Our analysis of CPD-56o 8032 gives the wind properties (T *=34500K, lg (L/L ⊙)=3.8, lg (M/M ⊙a−1)=−5.4,v ∞=225 km s−1) and chemistry (C/He=0.5, O/He=0.1, by number), the latter suggesting an intimate relationship with the Ovi PN central stars and the PG 1159-035 objects. A comparison between the wind properties of CPD-56o 8032 and Sk-66o 40 (WN 10) indicates that low excitation, low wind velocity WR winds are common to both low mass PN central stars (WC sequence) and high mass post-LBV's (WN sequence).
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Aitken D.K., Barlow M.J., Roche, P.F., Spenser, P.M., 1980,MNRAS 192, 679
Barlow M.J., Storey P.J., 1993, in Proc. IAU Symp. 155,Planetary Nebulae, Kluwer, p. 92
Cowley A.P., Hiltner W.A., 1969,A&A 3, 372
Crowther P.A., Hillier, D.J., Smith, L.J., 1995,A&A 293, 172
Hillier D.J., 1989,ApJ 347, 392
Hiller D.J., 1990,A&A 231, 111
Pollacco, D.L., Kilkenny, D., Marang, F., van Wyk, F., Roberts, G., 1992,MNRAS 256, 669
Webster B.L., Glass I.S., 1974,MNRAS 166, 491
Wood P.R., Faulkner D.J., 1986,ApJ 307, 659
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Crowther, P.A., De Marco, O., Barlow, M.J. et al. A quantitative analysis of the prototype [WCL] star CPD-56° 8032. Astrophys Space Sci 238, 119–123 (1996). https://doi.org/10.1007/BF00645506
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DOI: https://doi.org/10.1007/BF00645506