Abstract
A quantitative model explaining a periodic wave-like variation in both the optical continuum and the emission line fluxes of the symbiotic binary V443 Her is presented. The model suggests that behaviour of spectrophotometric parameters is caused by a different projection of the circumstellar matter located mostly between the components of the binary, viewing the system at different orbital phases. Our model suggests that the inclination of the orbit is 18° (+12°, −3°) and the mass ratio of the cool to the hot component is 2(+1). It is shown that the previous interpretation in terms of a reflection effect is incorrect.
Similar content being viewed by others
References
Archipova, V.P. and Noskova, P.I.: 1988a,Pisma v AZh 14, 445.
Archipova, V.P. and Noskova, P.I.: 1988b,Pisma v AZh 14, 510.
Archipova, V.P., Ikonnikova, N.P. and Noskova, P.I.: 1995,Pisma v AZh 21, 379.
Belyakina, T.S.: 1970,Astrofizika 6, 49.
Belyakina, T.S.: 1992,Izv. Krym. Astofiz. Obs. 84, 49.
Boyarchuk, A.A.: 1966,AZh 43, 976.
Dobrzycka, D., Kenyon, S.J. and Mikołajewska, J.: 1993,Astron. J. 106, 284 (DKM).
Formiggini, L. and Leibowitz, E.M.: 1990,Astron. Astrophys. 227, 121.
Garcia, M.R. and Kenyon, S.J.: 1988, In: Mikołajewska et al (eds.),The Symbiotic Phenomenon, IAU Coll. No. 103, Kluwer Acad. Press, Dordrecht, p. 27.
Hadrava, P.: 1992,Astron. Astrophys. 257, 218.
Horne, K. and Marsh, T.R.: 1986,Mon. Not. R. Astron. Soc. 218, 761.
Kenyon, S.J.: 1982,Publ. Astron. Soc. Pacific 94, 165.
Kenyon, S.J.: 1986,The Symbiotic Stars, Cambridge Univ. Press. p. 27.
Kenyon, S.J. and Bateson, F.M.: 1984,Publ. Astron. Soc. Pacific 96, 321.
Kenyon, S.J. and Fernandez-Castro, T.: 1987,Astron. J. 93, 938.
Kenyon, S.J., Oliversen, N.A., Mikołajewska, J., Mikołajewski, M., Stencel, R.E., Garcia, M.R. and Anderson, C.M.: 1991,Astron. J. 101, 637.
Kolotilov, E.A., Munari, U. and Yudin, B.F.: 1995,Astron. Astrophys. 293, 815 (KMY).
Munari, U.: 1988,Astron. Astrophys. 207, L8.
Munari, U.: 1992,Astron. Astrophys. 257, 163.
Munari, U. and Buson, L.M.: 1992,Astron. Astrophys. 255, 158.
Mürset, U., Nussbaumer, H., Schmid, H.M. and Vogel, M.: 1991,Astron. Astrophys. 248, 458.
Schmutz, W., Schild, H., Mürset, U. and Schmid, H.M.: 1994,Astron. Astrophys. 288, 819.
Seaquist, E.R., Taylor, A.R. and Button, S.: 1984,Astrophys. J. 284, 202 (STB).
Sion, E.M. and Ready, Ch.J.: 1992,Publ. Astron. Soc. Pacific 104, 87.
Skopal, A.: 1994,Astron. Astrophys. 286, 453.
Skopal, A.: 1996,Astron. Astrophys. (in press).
Skopal, A., Chochol, D., Vittone, A., Blanco, C. and Mammano, A.: 1991,Astron. Astrophys. 245, 531.
Skopal, A., Hric, L., Urban, Z., et al.: 1992,Contrib. Astron. Obs. Skalnaté Pleso 22, 131.
Skopal, A., Vittone, A. and Errico, L.: 1993,Astrophys. Space Sci. 209, 79 (SVE93).
Solf, J.: 1983,Astrophys. J. Lett. 266, L113.
Solf, J.: 1987,Astron. Astrophys. 180, 213.
Taranova, O.G. and Yudin, B.F.: 1987,Astron. Tsirk. 1489, 7.
Tiff, W.G. and Greenstein, J.L.: 1958,Astrophys. J. 127, 160.
Vogel, M.: 1993,Astron. Astrophys. 274, L21.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Skopal, A. Circumstellar material in the symbiotic binary V443 herculis. Astrophys Space Sci 238, 285–302 (1996). https://doi.org/10.1007/BF00641693
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1007/BF00641693