Skip to main content
Log in

AGB stars in the Magellanic Clouds

  • III. Late Type Stars
  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

The stars that will be detectable in the Magellanic Clouds by the DENIS and 2MASS near infrared surveys are enumerated. All thermally-pulsing AGB stars will be observable in I, J, H and K, along with the top two magnitudes of both the early-AGB and the first giant branch. All carbon stars will be visible, and normal (N type) C stars will be easily distinguished by their large J-K colours. However, it will not be possible to separate faint, warm C stars from K and M stars using the photometry alone. Photometry of AGB stars in clusters will allow an accurate evaluation of the AGB tip luminosities as a function of initial mass. Random phase K magnitudes of LPVs and Cepheids should provide a better measure of the LMC tilt and distortions in the SMC. The K survey should turn up 100 to 150 objects undergoing superwind mass loss, these objects being OH/IR stars and the dust-enshrouded C star equivalents of OH/IR stars. It is shown that crowding should not be a problem even in the LMC bar.

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

Access this article

Subscribe and save

Springer+ Basic
$34.99 /Month
  • Get 10 units per month
  • Download Article/Chapter or eBook
  • 1 Unit = 1 Article or 1 Chapter
  • Cancel anytime
Subscribe now

Buy Now

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Bertelli, G., Mateo, M., Chiosi, C. and Bressan, A.: 1992,Astrophysical Journal 388, 400

    Google Scholar 

  • Bessell, M.S. and Brett, J.M.: 1988,Publications of the ASP 100, 1134

    Google Scholar 

  • Bessell, M.S. and Wood, P.R.: 1984,Publications of the ASP 96, 247

    Google Scholar 

  • Bessell, M.S., Wood, P.R. and Lloyd Evans, T.: 1983,Monthly Notices of the RAS 202, 59

    Google Scholar 

  • Blanco, V.M. and McCarthy, M.F.: 1983,Astronomical Journal 88, 1442

    Google Scholar 

  • Chiosi, C., Wood, P.R. and Capitanio, N.: 1993,Astrophysical Journal, Supplement Series 86, 541

    Google Scholar 

  • Demers, S., Irwin, M.J. and Kunkel, W.E.: 1993,Monthly Notices of the RAS 260, 103

    Google Scholar 

  • Feast, M.W., Glass, I.S., Whitelock, P.A., and Catchpole, R.M.: 1989,Monthly Notices of the RAS 241, 375

    Google Scholar 

  • Frogel, J.A. and Blanco, V.M.: 1990,Astrophysical Journal 365, 168

    Google Scholar 

  • Frogel, J.A., Mould, J. and Blanco, V.M.: 1990,Astrophysical Journal 352, 96

    Google Scholar 

  • Glass, I.S. and Reid, N.: 1985,Monthly Notices of the RAS 214, 405

    Google Scholar 

  • Hodge, P.W. and Wright, F.W. 1967,The Large Magellanic Cloud, (Smithsonian Press: Washington,D.C.)

    Google Scholar 

  • Hodge, P.W. and Wright, F.W. 1977,The Small Magellanic Cloud, (University of Washington Press: Seattle)

    Google Scholar 

  • Hughes, S.M.G.: 1989,Astronomical Journal 97, 1634

    Google Scholar 

  • Hughes, S.M.G. and Wood, P.R.: 1990,Astronomical Journal 99, 784

    Google Scholar 

  • Hughes, S.M.G., Wood, P.R. and Reid, N.: 1991,Astronomical Journal 101, 1304

    Google Scholar 

  • Jura, M. and Kleinmann, S.G.: 1992,Astrophysical Journal, Supplement Series 79, 105

    Google Scholar 

  • Reid, N.: 1991,Astrophysical Journal 382, 143

    Google Scholar 

  • Reid, N., Glass, I.S. and Catchpole, R.M.: 1988,Monthly Notices of the RAS 232, 53

    Google Scholar 

  • Reid, N. and Mould, J.: 1990,Astrophysical Journal 360, 490

    Google Scholar 

  • Reid, N., Mould, J. and Thompson, I.: 1987,Astrophysical Journal 323, 433

    Google Scholar 

  • van den Bergh, S.: 1981,Astronomy and Astrophysics, Supplement Series 46, 79

    Google Scholar 

  • Vassiliadis, E. and Wood, P.R.: 1993,Astrophysical Journal 413, 641

    Google Scholar 

  • Welch, D.L., McLaren, R.A., Madore, B.F. and McAlary, C.W.: 1987,Astrophysical Journal 321, 162

    Google Scholar 

  • Westerlund, B.E., Azzopardi, M., Breysacher, J. and Rebeirot, E.: 1992,Astronomy and Astrophysics 260, L4

    Google Scholar 

  • Wood, P.R. 1990, inFrom Miras to Planetary Nebulae, eds. M.O. Mennessier and A. Omont (Editions Frontieres: Gif sur Yvette), p.67

    Google Scholar 

  • Wood, P.R., Bessell, M.S. and Fox, M.W.: 1983,Astrophysical Journal 272, 99

    Google Scholar 

  • Wood, P.R., Bessell, M.S. and Paltoglou, G.: 1985,Astrophysical Journal 290, 477

    Google Scholar 

  • Wood, P.R. and Cahn, J.H.: 1977,Astrophysical Journal 211, 499

    Google Scholar 

  • Wood, P.R., Whiteoak, J.B., Hughes, S.M.G., Bessell, M.S., Gardner, F.F. and Hyland, A.R.: 1992,Astrophysical Journal 397, 552

    Google Scholar 

  • Wright, F.W. and Hodge, P.W.: 1971,Astronomical Journal 76, 1003

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Wood, P.R. AGB stars in the Magellanic Clouds. Astrophys Space Sci 217, 121–130 (1994). https://doi.org/10.1007/BF00990037

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00990037

Key words