No CrossRef data available.
Article contents
Mass near the Sun
Published online by Cambridge University Press: 25 May 2016
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.
I review the dynamical measurements of mass in the solar neighborhood and show that, within 1 kpc, ∼ 40% is unaccounted for by known stars and gas. I discuss several interpretations of the data including the ‘standard model’ where the extra mass is due to a spherical dark halo. I argue that the evidence for a radically different picture of an ultra-flat distribution is at least as compelling as the standard model.
- Type
- Chapter 8: How do we put it together?
- Information
- Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 651 - 659
- Copyright
- Copyright © Kluwer 1996
References
Udalski, A.
Szymański, J., Kaluzny, J., Kubiak, M., Krzeminiński, W., Mateo, M., Preston, G. W., & Paczyński, B.
1993, Acta Astron., 43, 289
Google Scholar