Advertisement

Astrophysics and Space Science

, Volume 118, Issue 1–2, pp 365–366 | Cite as

Expected and observed late giant star counts in the Milky Way bulge

  • V. M. Blanco
  • B. M. Blanco
Section 4a: Compact Stars, and Galactic Structure

Abstract

In this paper, late M giants star counts in the Milky Way central bulge are compared with those expected from the Hubble and de Vaucouleurs surface brightness distributions.

Keywords

Surface Brightness Brightness Distribution Giant Star Central Bulge Star Count 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

References

  1. Bahcall, J. and Soneira, R.: 1980,Astrophys. J. Suppl. 44, 73.Google Scholar
  2. Blanco, V. M., McCarthy, M. F., and Blanco, B. M.: 1984,Astron. J. 89, 636.Google Scholar
  3. de Vaucouleurs, G.: 1953,Monthly Notices Roy. Astron. Soc. 113, 134.Google Scholar
  4. de Vaucouleurs, G. and Pence, W. D.: 1978,Astron. J. 83, 1163.Google Scholar
  5. Hidayat, B. and Blanco, V. M.: 1968,Astron. J. 73, 712.Google Scholar
  6. Hubble, E.: 1930,Astrophys. J. 71, 231.Google Scholar
  7. Mikami, T., and Ishida, K.: 1981,Publ. Astron. Soc. Japan 33 135.Google Scholar
  8. Morgan, W. W. and Mayall, N. U.: 1957,Publ. Astron. Soc. Pacific 69, 291.Google Scholar
  9. Morgan, W. W., and Osterbrock, D. E.: 1969,Astron. J. 74, 15.Google Scholar
  10. Nassau, J. J. and Blanco, V. M.: 1958,Astrophys. J. 128, 46.Google Scholar
  11. Whitford, A. E.: 1978,Astrophys. J. 226, 777.Google Scholar
  12. Young, S.: 1976,Astron. J. 81, 807.Google Scholar

Copyright information

© D. Reidel Publishing Company 1986

Authors and Affiliations

  • V. M. Blanco
    • 1
  • B. M. Blanco
    • 1
  1. 1.Cerro Tololo Inter-American ObservatoryNational Optical Astronomy ObservatoriesLa SerenaChile

Personalised recommendations