Abstract
Space densities and galacticz-distributions of novae, recurrent novae, dwarf novae and symbiotic stars are newly determined and discussed in the context of earlier determinations. The data are then compared with the distributions of single and binary stars of possibly related types (late type giants, Mira variables, Algol systems, W UMa systems).
Novae and dwarf novae have similar distributions, those of fairly young stellar populations. The observed space density of potential novae (novalike objects) indicates that the mean recurrence time of novae might be as small as a few hundred years, which leads, with given nova shell masses and mass transfer rates in the minimum stage, to a secular decrease of the masses of the components undergoing nova outbursts.
Recurrent novae and symbiotic stars have distributions of older stellar populations, similar to those of late type giants and Mira variables.
On the basis of galactic distribution, novae and dwarf novae are closely related and may be final stages of W UMa systems, as well as progenitors of supernovae of type I. A small fraction of W UMa systems seems to belong to an older population. If evolutionary transitions between these types of stars can be substantiated, the presence of a minority of novae and dwarf novae in globular clusters and of supernovae I in elliptical galaxies can be explained.
Due to the lack of sufficiently well determined space distributions of Algol binaries, the suggestion that long-period Algol systems might be the progenitors of cataclysmic binaries can as yet neither be substantiated nor refuted. A very high space density of long-period Algol systems in the solar neighbourhood is derived. The observed space density of cataclysmic binaries could be explained by the transformation of a small percentage of the long-period Algol systems by common envelope evolution.
Similar content being viewed by others
References
Allen, C. W.: 1954,Monthly Notices Roy. Astron. Soc. 114, 387.
Allen, C. W.: 1973,Astrophysical Quantities, 3rd edition (and previous editions). Athlone Press, London.
Allen, D. A.: 1979, in F. M. Batesonet al. (eds.), ‘Changing Trends in Variable Star Research’,IAU Colloq. 46, 125.
Allen, D. A.: 1980,Monthly Notices Roy. Astron. Soc. 192, 521.
Baade, W.: 1958, in D. J. K. O'Connell (ed.), ‘Stellar Populations’,Ric. Astron. Spec. Vatican 5, 165.
Bailey, J.: 1981,Monthly Notices Roy. Astron. Soc. 197, 31.
Barlow, M. J., Brodie, J. P., Brunt, C. C., Hanes, D. A., Hill, P. W., Mayo, S. K., Pringle, J. E., Ward, M. J., Watson, M. G., Whelan, J. A. J., and Willis, A. J.: 1981,Monthly Notices Roy. Astron. Soc. 195, 61.
Batten, A. H., Fletcher, J. M., and Mann, P. J.: 1978,Publ. Dominion Astrophys. Obs. Victoria 15, 121.
Bruch, A.: 1982, Ph.D. thesis, Münster University.
Bruch, A., Duerbeck, H. W., and Seitter, W. C.: 1981,Mitt. Astron. Ges. 52, 34.
Budding, E.: 1983,Astrophys. Space Sci. 99, (this issue).
Cahn, J. H. and Wyatt, S. P.: 1978, in Y. Terzian (ed.), ‘Planetary Nebulae’IAU Symp. 76, 3.
Dinerstein, H. and Hoffleit, D.: 1973,Inf. Bull. Var. Stars, No. 845.
Duerbeck, H. W.: 1980, Habilitation thesis, Bonn.
Duerbeck, H. W.: 1981,Publ. Astron. Soc. Pacific 93, 165.
Duerbeck, H. W. and Seitter, W. C.: 1979,ESO Messenger 17, 1; see alsoMitt. Astron. Ges. 50, 90 (1980).
Duerbeck, H. W. and Seitter, W. C.: 1982, in K. Schaifers and H. H. Voigt (eds.),Landolt-Börnstein N.S. VI/2, 197.
Eggleton, P. P.: 1983, in M. Livio and G. Shaviv (eds.), ‘Cataclysmic Variables and Related Objects’,IAU Colloq. 72, 239.
Eggleton, P. P., Mitton, S., and Whelan, J. A. J. (eds.): 1976, in ‘Structure and Evolution of Close Binary Stars’,IAU Symp. 73.
Garrison, R. F., Hiltner, W. A., and Schild, R. E.: 1982,IAU Circ., No. 3730.
Hoffmann, M.: 1983, private communication.
Hudec, R.: 1981,Bull. Astron. Inst. Czech. 32, 93.
Iwanowska, W. and Burnicki, A.: 1962,Bull. Acad. Pol. Sci. Ser. Sci. Math. Astron. Phys. 10 (10), 537.
Johnson, H. M. and MacLeod, J. M.: 1963,Publ. Astron. Soc. Pacific 75, 123.
Kamper, K. W.: 1979, in H. M. van Horn and V. Weidemann (eds.), ‘White Dwarfs and Variable Degenerate Stars’,IAU Colloq. 53, 494.
Kholopov, P. N.: 1981,Perem. Zvezdy 21, 465.
Kopylov, I. M.: 1957, in G. H. Herbig (ed.), ‘Non-Stable Stars’,IAU Symp. 3, 71.
Kraft, R. P.: 1962,Astrophys. J. 135, 408.
Kraft, R. P.: 1965,Astrophys. J. 142, 1588.
Kraft, R. P.: 1967,Publ. Astron. Soc. Pacific 79, 395.
Kraft, R. P. and Luyten, W.: 1965,Astrophys. J. 142, 1041.
Kukarkin, B. W.: 1954,Untersuchung der Struktur und Entwicklung der Sternsysteme auf der Grundlage des Studiums veränderlicher Sterne, Akademie-Verlag, Berlin.
Law, W. Y. and Ritter, H.: 1983,Astron. Astrophys. 123, 33.
Margon, B., Downes, R. A., and Gunn, J. E.: 1981,Astrophys. J. 247, L89.
Mayall, M. W.: 1949,Publ. Astron. Soc. Pacific 54, 191.
Meyer-Hofmeister, E.: 1982, in K. Schaifers and H. H. Voigt (eds.),Landolt-Börnstein N.S. VI/2b, 152.
Mikami, T. and Ishida, K.: 1981,Publ. Astron. Soc. Japan 33, 135.
Moffat, A. F.: 1982, private communication.
Neckel, Th.: 1967,Veröff. Landssternwarte Heidelberg 19.
Neckel, Th. and Klare, G.: 1980,Astron. Astrophys. Suppl. 42, 251.
Oort, J. H.: 1958, in D. J. K. O'Connell (ed.), ‘Stellar Populations’,Ric. Astron. Spec. Vatican. 5, 415.
Paczynski, B.: 1976, in P. Eggleton, S. Mitton, and J. A. J. Whelan (eds.), ‘Structure and Evolution of Close Binary Systems’,IAU Symp. 73, 27.
Paczynski, B.: 1980, in P. A. Weyman (ed.),Highlights of Astronomy 5 D. Reidel Publ. Co., Dordrecht, Holland, p. 27.
Parenago, P. P.: 1955, in ‘Principes fondamentaux de classification stellaire’,Colloque International du CNRS, CNRS, Paris, p. 13.
Payne-Gaposchkin, C. H.: 1977, in M. Friedjung (ed.),Novae and Related Stars, D. Reidel Publ. Co., Dordrecht, Holland, p. 3.
Plaut, L.: 1965, in A. Blaauw and M. Schmidt (eds.),Stars and Stellar Systems V, University of Chicago Press, Chicago, p. 311.
Popov, M. V.: 1964,Perem. Zvezdy 15, 115.
Primkulov, Sh.: 1968,Tsirk. Astron. Tashkent 8, No. 255.
Richter, G.: 1968,Veröffentl. Sternw. Sonneberg 7, 229.
Richter, G.: 1983,Inf. Bull. Var. Stars, No. 2267.
Ritter, H.: 1976,Monthly Notices Roy. Astron. Soc. 175, 279.
Ritter, H.: 1983,Catalogue of Cataclysmic Binaries, MPI Astrophysik Garching, (MPA-51).
Robinson, E. L.: 1975,Astron. J. 80, 515.
Rosino, L.: 1973,Astron. Astrophys. Suppl. 9, 347.
Rudak, B.: 1982, in M. Friedjung and R. Viotti (eds.), ‘The Nature of Symbiotic Stars’,IAU Colloq. 70, 275.
Sahade, J.: 1959, Liège Symp. No. 9, ‘Modèles d'étoiles et évolution stellaire’,Mém. Soc. R. Liège Sér. 5, t. 3, p. 76.
Sawyer, H.: 1938,J. Roy. Astron. Soc. Canada 32, 69.
Sawyer-Hogg, H. and Wehlau, A.: 1964,J. Roy. Astron. Soc. Can. 58, 163.
Scheffler, H.: 1983, in K. Schaifers and H. H. Voigt (eds.),Landolt-Börnstein N.S. VI/2c, 175.
Schmidt-Kaler, Th.: 1957,Z. Astrophys. 41, 182.
Schmidt-Kaler, Th.: 1962,Kl. Veröffentl. Remeis-Sternw. Bamberg 34, 109.
Schmidt-Kaler, Th.: 1982, in K. Schaifers and H. H. Voigt (eds.),Landolt-Börnstein N. S. VI/2b, 1.
Shapley, H.: 1948,Harvard Obs. Monograph 7, 249.
Shu, F. H.: 1980, in M. J. Plavec, D. M. Popper, and R. K. Ulrich (eds.), ‘Close Binary Stars: Observations and Interpretation’,IAU Symp. 88, 477.
Smak, J.: 1982,Acta Astron. 32, 213.
Starrfield, S., Truran, J. W., and Sparks, W. M.: 1981,Astrophys. J. 243, L27.
Svetchnikov, M. A., Istomin, L. F., and Grehova, O. A.: 1980,Perem. Zvezdy 21, 399.
Trimble, V.: 1983,Nature 303, 137.
Tsvetkov, D. Yu.: 1981,Soviet Astron. Letters 7, 254.
Upgren, A. R.: 1963,Astron. J. 68, 475.
Van't Veer, F.: 1975,Astron. Astrophys. 40, 167.
Vasilevskis, S., Harlan, E. A., Klemola, A. R., and Wirtanen, C. A.: 1975,Publ. Lick Obs. 22, Pt. 5.
Vidal, N. V. and Rodgers, A. W.: 1974,Publ. Astron. Soc. Pacific 86, 26.
Vilhu, O.: 1981,Astrophys. Space Sci. 78, 401.
Voikhanskaya, N. F.: 1973,Astrofiz. Issled 5, 89.
Vogt, N.: 1981, Habilitation thesis, Bochum University.
Wallerstein, G.: 1981,Observatory 101, 172.
Warner, B.: 1974a,Monthly Notices Roy. Astron. Soc. 167, 61p.
Warner, B.: 1974b,Monthly Notices Astron. Soc. Southern Africa 33, 21.
Webbink, R. F.: 1976,Astrophys. J. 209, 829.
Webbink, R. F.: 1978,Publ. Astron. Soc. Pacific 90, 57.
Webbink, R. F.: 1980, in M. J. Plavec, D. M. Popper, and R. K. Ulrich (eds.), ‘Close Binary Stars: Observations and Interpretation’,IAU Symp. 88, 561.
Wenzel, W. and Meinunger, I.: 1978,Astron. Nachr. 299, 237.
Yungelson, L. R.: 1982, in J. Tremko (ed.),Ejection and Accretion of Matter in Binary Systems, Veda, Bratislava, p. 11.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Duerbeck, H.W. Constraints for cataclysmic binary evolution as derived from space distributions. Astrophys Space Sci 99, 363–385 (1984). https://doi.org/10.1007/BF00650260
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00650260