Abstract
Recent Hα spectroscopy of the helium-strong star δ Ori C (= HD 36485) has revealed the presence of double-peaked Hα emission in this sharp-lined and strongly magnetic B3V star. Changes in the emission are evident over a 3.5 hr time span, and the profile variations are periodic with a period on the order of 1 d. 5
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Barker, P.K., Brown, D.N., Bolton, C.T., and Landstreet, J.D. 1982, in Advances in Ultraviolet Astronomy: Four Years of IUE Research, ed. Y. Kondo, J.M. Mead, and R.D. Chapman (NASA CP-2238), p. 589.
Bohlender, D.A. 1989, Ap.J., 346, 459.
Bohlender, D.A., Brown, D.N., Landstreet, J.D., and Thompson, I.B. 1987, Ap.J., 323, 325.
Bolton, C.T., Fullerton, A.W., Bohlender, D.A., Landstreet, J.D., and Gies, D.R. 1986, in IA U Colloquium 92, The Physics of Be Stars, ed. A. Slettebak and T.P. Snow (Cambridge: Cambridge University Press), p. 82.
Drake, S.A., Abbott, D.C., Bastian, T.S., Bieging, J.H., Churchwell, E., Dulk, G., and Linsky, J.L. 1987, Ap.J., 322, 902.
Drilling, J.S., and Hill, P.W. 1986, in Hydrogen Deficient Stars and Related Objects, eds. K. Hunger et al. (Dordrecht: Reidel) p. 499.
Hunger, K., Heber, U., and Groote, D. 1989, Asiron. Astrophys., 224, 57.
Shore, S.N., and Brown, D.N. 1990, Ap.J., 365, 665.
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© 1992 Springer-Verlag
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Bohlender, D.A., Bolton, C.T., Walker, G.A.H. (1992). Variable Hα emission in the helium-strong star δ orionis C. In: Heber, U., Jeffery, C.S. (eds) The Atmospheres of Early-Type Stars. Lecture Notes in Physics, vol 401. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-55256-1_309
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DOI: https://doi.org/10.1007/3-540-55256-1_309
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