Hostname: page-component-5c6d5d7d68-qks25 Total loading time: 0 Render date: 2024-08-22T02:41:05.626Z Has data issue: false hasContentIssue false
  • English
  • Français

Link between Mass-Loss and Variability Type for AGB Stars?

Published online by Cambridge University Press:  12 April 2016

Željko Ivezić  and
Gillian R. Knapp
Željko Ivezić
Affiliation:
Princeton University, Department of Astrophysical Sciences, Princeton, NJ 08544-1001, USA
Gillian R. Knapp
Affiliation:
Princeton University, Department of Astrophysical Sciences, Princeton, NJ 08544-1001, USA

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.

We discuss difficulties in explaining the distribution of AGB stars in the 25–12 vs. 12–K color–color diagram by steady-state radiatively driven models, and propose that the discrepancy may be due to changes of mass-loss rate with the time scales of ∼ 100 yr.

Type
Part 2. Variability of High-Luminosity Stars
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 124
Copyright
Copyright © Astronomical Society of the Pacific 2000