Skip to main content

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 283))

  • 187 Accesses

Abstract

I present some new results on mass-losing and pulsating stars in the LMC and SMC, based on an analysis of OGLE/MACHO light curves and DENIS/2MASS/ISO infrared data, for samples of AGB stars detected by IRAS, and by the recent ISOCAM “minisurvey” of the SMC

The conclusions are that (1) the scatter in the PL-relation at long periods is (much) larger than that for P < 400 days, (2) the SEDs of some carbon stars are not well fitted in the blue, indicating possibly some missing opacity problem in the model atmospheres, or that the effective temperatures are below 2600 K, the lowest temperature in the available model grid, and (3) the period-mass loss rate relation for C-rich SMC stars seems to follow that derived for Galactic carbon-rich Miras, suggesting no explicit dependence of mass loss rate on metallicity

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 129.00
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 169.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book
USD 169.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

Download references

Author information

Authors and Affiliations

Authors

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 2003 Springer Science+Business Media Dordrecht

About this chapter

Cite this chapter

Groenewegen, M. (2003). Mass-Losing and Pulsating AGB Stars in the Magellanic Clouds. In: Nakada, Y., Honma, M., Seki, M. (eds) Mass-Losing Pulsating Stars and their Circumstellar Matter. Astrophysics and Space Science Library, vol 283. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0139-7_11

Download citation

  • DOI: https://doi.org/10.1007/978-94-010-0139-7_11

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-3968-0

  • Online ISBN: 978-94-010-0139-7

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics