Hostname: page-component-6bf8c574d5-mcfzb Total loading time: 0 Render date: 2025-03-09T14:21:15.337Z Has data issue: false hasContentIssue false
  • English
  • Français

Do Halo Red Giant Stars Contribute to the High-Velocity Gas Falling onto the Milky Way Disk?

Published online by Cambridge University Press:  26 May 2016

Klaas S. de Boer
Klaas S. de Boer*
Affiliation:
Sternwarte der Universität Bonn, D-53121 Bonn, Germany

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.

The amount of gas shed by red giant stars in the halo is assessed to find its contribution to the long known infall of high-b gas. The infall rate due to RG star mass loss equals 3 · 10−6 M⊙ kpc−1 y−1.

Type
Part 2. Origin
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 170 - 171
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Altmann, M., Edelmann, H., & de Boer, K.S. 2003, A&A, submitted.Google Scholar
Audouze, J., & Tinsley, B.M. 1976, ARA&A, 12, 43.Google Scholar
de Boer, K.S. 1985, A&A 142, 321.Google Scholar
de Boer, K.S., Aguilar Sánchez, Y., Altmann, M., Geffert, M., Odenkirchen, M., Schmidt, J.H.K., & Colin, J. 1997, A&A 327, 587.Google Scholar
Downes, R.A. 1986, ApJS 61, 569.Google Scholar
Oort, J.H. 1966, Bull. Astron. Inst. Neth., 18, 421.Google Scholar
Pagel, B.E.J. 1997, ‘Nucleosynthesis and chemical evolution of galaxies’, Cambridge Univ. press.Google Scholar