Hostname: page-component-77c89778f8-fv566 Total loading time: 0 Render date: 2024-07-19T15:29:05.843Z Has data issue: false hasContentIssue false
  • English
  • Français

Photometric Investigation of Visual Binaries with a Component above the Main Sequence

Published online by Cambridge University Press:  12 April 2016

O.G. Franz
O.G. Franz*
Affiliation:
Lowell Observatory, Flagstaff, Arizona 86002, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Visual binaries containing a component above the main sequence in combination with a main-sequence star provide an excellent opportunity for determining absolute magnitudes of evolved stars. Some aspects of this technique are discussed, and preliminary results are presented.

Type
Part II: Evolutionary Trends in Wide Binary Systems
Information
International Astronomical Union Colloquium , Volume 69: Binary and Multiple Stars as Tracers of Stellar Evolution , 1982 , pp. 123 - 128
Copyright
Copyright © Reidel 1982

References

Abt, H.A.: 1981, Astrophys. J. Suppl. 45, pp. 437–456.Google Scholar
Aitken, R.G.: 1932, New General Catalogue of Double Stars, Carnegie Institution of Washington.Google Scholar
Allen, C.W.: 1973, Astrophysioal Quantities, University of London, The Athlone Press.Google Scholar
Bidelman, W.P.: 1954, Astrophys. J. Suppl. 1, pp. 175–267.Google Scholar
Bidelman, W.P.: 1958, Pubi. Astron. Soc. Pacific 70, pp. 168–179.Google Scholar
Culver, R.B., Ianna, P.A., and Franz, O.G.: 1977, Pubi. Astron. Soc. Pacific 89, pp. 397–399.Google Scholar
Eggen, O.J.: 1956, Astron. J. 61, pp. 361–380.Google Scholar
Eggen, O.J.: 1963, Astron. J. 68, pp. 483–514.Google Scholar
Eggen, O.J.: 1965, Astron. J. 70, pp. 19–93.Google Scholar
Franz, O.G.: 1966, Lowell Obs. Bull. 6, pp. 251–256.Google Scholar
Franz, O.G.: 1970, Lowell Obs. Bull. 7, pp. 191–197.Google Scholar
Jeffers, H.M., van den Bos, W.H., and Greeby, F.M.: 1963, Pubi. Lick Obs. 21.Google Scholar
Johnson, H.L.: 1953, Astrophys. J., 117, pp. 361–365.Google Scholar
Leonard, F.C.: 1921, Publ. Astron. Soc. Pacific 33, pp. 213–214 (abstract).Google Scholar
Leonard, F.C.: 1923, Lick. Obs. Bull. 10, pp. 169–194.Google Scholar
Rakos, K.D.: 1965, Applied Optics 4, pp. 1453–1456.Google Scholar
Slettebak, A.: 1963, Astrophys. J. 138, pp. 118–139.Google Scholar
Stephenson, C.B.: 1960, Astron. J. 65, pp. 60–79.Google Scholar
Stephenson, C.B., and Sanwal, N.B.: 1969, Astron. J. 74, pp. 689–704.Google Scholar
Wallenquist, Â.: 1954, Ann. Uppsala Astron. Obs. 4, No. 2, pp. 1–79.Google Scholar
White, N.M.: 1981, private communication.Google Scholar
White, N.M., and Wing, R.F.: 1978, Astrophys. J. 222, pp. 209–219.Google Scholar