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The Stellar Distribution above the Galactic Plane: An Introduction

Published online by Cambridge University Press:  30 March 2016

Ivan R. King
Ivan R. King*
Affiliation:
Astronomy Department, University of California, Berkeley

Extract

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This paper will truly be an introduction — a presentation and a discussion of the basic problems, to set the stage for detailed research results that will be reported by others.

The problem of star distribution perpendicular to the galactic plane has one central theme, which can be played in two modes. The theme is the drop-off of star-density with z, and the two modes are the general density profile and the stratification of populations. (This last phrase is a convenient one, but I should warn against taking it too literally. By “stratification” I mean a gradual change, rather than a sharp separation; and I want to emphasize even more strongly that the word “population” should be used in a general and abstract sense, rather than as a sharp separation into two, or five, or any other discrete number of components.)

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 4 , Issue 2: Highlights of Astronomy. As presented at the XVIth General Assembly of the IAU, 1976 (Part II) , 1977 , pp. 41 - 48
Copyright
Copyright © Reidel 1977

References

Faber, S. M., Burstein, D., Tinsley, B., and King, I. R.: 1976, Astron. J. 81, 45.Google Scholar
Hill, E. R.: 1960, Bull. Astron. Inst. Neth. 15, 1 (No. 494).Google Scholar
Luyten, W. J.; 1960, ‘A Search for Faint Blue Stars. XXII. The Star Density in High Galactic Latitude,’ University of Minnesota.Google Scholar
Luyten, W. J.: 1968, Monthly Notices Roy. Astron. Soc. 139, 221.Google Scholar
Murray, C. A., and Sanduleak, N.: 1972, Monthly Notices Roy. Astron. Soc. 157, 273.CrossRefGoogle Scholar
Oort, J. H.: 1932, Bull. Astron. Inst. Neth. 6, 249 (No. 238).Google Scholar
Oort, J. H.: 1960, Bull. Astron. Inst. Neth. 15., 45 (No. 494).Google Scholar
Oort, J. H.: 1965, in A., Blaauw and M., Schmidt (eds.), Galactic Structure, University of Chicago Press, Chicago, Ch. 21.Google Scholar
Ostriker, J. P., and Peebles, P. J. E.: 1973, Astrophys. J. 186, 467.Google Scholar
Sanduleak, N.: 1965, ‘The Luminosity Function of the M Dwarf Stars,’ Case Institute of Technology (Ph.D. thesis).Google Scholar
Sanduleak, N.: 1976, Astron. J. 81, 350.Google Scholar
Schmidt, M.: 1975, Astrophys. J. 202, 22.CrossRefGoogle Scholar
Weistrop, D.: 1972a, Astron. J. 77, 366.CrossRefGoogle Scholar
Weistrop, D.: 1972b, Astron. J. 77, 849.Google Scholar
Weistrop, D.: 1976a, Astrophys. J. 204, 113.CrossRefGoogle Scholar
Weistrop, D.: 1976b, Astron. J. 81 (in press).Google Scholar