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K giants and the total amount of matter near the sun

Bahcall, J. N.·1984·The Astrophysical Journal

Abstract

The Poisson and Boltzmann equations are solved numerically for realistic Galaxy models which include multiple disk components (between 14 and 28), a Population II spheroid, and an unseen massive halo. As a guide in constructing the theoretical models, a population of normal-metallicity (disk) K giants is isolated using existing data and is shown to be well described by an isothermal distribution function with a velocity dispersion perpendicular to the plane of 20 km s-1. The total amount of matter in the vicinity of the Sun is determined by comparing the observed distributions of K giants with the predictions of detailed Galaxy models. The volume density of unobserved material near the Sun is about 0.1 M_sun; pc-3; the corresponding column density is about 30 M_sun; pc-2.

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Metadata

Authors
Bahcall, J. N.
Venue
The Astrophysical Journal
Published
1984-12
Volume
287
Pages
926
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2091570817
Cited by
160
References
0
FWCI
18.25
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: K giants and the total amount of matter near the sun. https://app.cochat.ai/papers/10.1086/162750
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Bahcall, J. N. (1984). K giants and the total amount of matter near the sun. The Astrophysical Journal. https://doi.org/10.1086/162750

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