Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-25T16:06:55.649Z Has data issue: false hasContentIssue false
  • English
  • Français

The Role of Space Observations in The Calibration of Fundamental Stellar Quantities

Published online by Cambridge University Press:  04 August 2017

Arthur D. Code
Arthur D. Code*
Affiliation:
Washburn Observatory, University of Wisconsin

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.

This paper summarizes the current status of ultraviolet spectrophotometry with emphasis on the instrumental characteristics unique to space observations and on the application of existing data to the calibration of stellar properties. The currently available data bases will be briefly reviewed. When combined with ground based data, ultraviolet observations provide information on effective temperatures and bolometric corrections for early type stars and on the nature of the intervening interstellar medium. The ultraviolet measurements are sensitive to chemical composition differences and provide a powerful tool in discussion of stellar evolution in composite systems. This review concludes with a brief discussion of future directions in instrumentation and analysis.

Type
1. Review Papers
Information
Symposium - International Astronomical Union , Volume 111: Calibration of Fundamental Stellar Quantities , 1985 , pp. 209 - 224
Copyright
Copyright © Reidel 1985 

References

Bohlin, R.C., Holm, A.V., Savage, B.D., Snijders, M.A.J., and Sparks, W.M. 1980, Astron. Astrophys., 85, 1.Google Scholar
Bohlin, R.C., and Holm, A.V. 1980, NASA IUE Newsletter No. 10, 37 Google Scholar
Brune, W.H., Mount, G.H., and Feldman, P.D. 1979, Astrophys. J., 227, 884.Google Scholar
Canfield, L.R., Johnston, R.G., and Madden, R.P. 1973, Appl. Optics, 12, 1611.Google Scholar
Carruthers, G.R., Heckathorn, H.M., and Opal, C.B. 1981, Astrophys. J., 243, 855.Google Scholar
Code, A.D. 1983, Adv. Space Res., 2, 119.CrossRefGoogle Scholar
Finley, D.S., Basri, G., and Bowyer, S. 1984, to be published in Proceedings of the Third Goddard IUE Symposium. Google Scholar
Harmer, D.L., Stickland, D. J., Lloyd, C., Harmer, C.F.W., Pike, C.D., and Corft, D. 1983, Mon. Not. R. Astron. Soc., 204, 927.CrossRefGoogle Scholar
Holberg, J.B., Forrester, W.T., and Shemansky, D.E. 1982, Astrophys. J., 257, 656.Google Scholar
Huenemoerder, D.P., de Boer, K.S., and Code, A.D., 1984, Astron. J., 89, 851.Google Scholar
Koornneef, J., Meade, M.R., Wesselius, P.R., Code, A.D., and van Duinen, R.J. 1982, Astron. Astrophys. Suppl., 47, 314.Google Scholar
Meyer, D.M., and Savage, B.D. 1981, Astrophys. J., 248, 545.Google Scholar
Polidan, R.S. and Holberg, J.B. 1985, in IAU Symposium No. 111: Calibration of Fundamental Stellar Quantities, eds. Hayes, D.S., Pasinetti, L.E. and Davis Philip, A.G. (Reidel: Dordrecht), p. 479.Google Scholar
Wesemael, F., Auer, L.H., Van Horn, H.M., and Savedoff, M.P. 1980, Astrophy. J. Suppl., 43, 159.Google Scholar
Wesselius, P.R., van Duinen, R.J., De Jonge, A.R.W., Aalders, J.W.G., Luinge, W., and Wildeman, K.J. 1982, Astron. Astrophys. Suppl., 49, 427.Google Scholar
Woods, T.N., Feldman, P.D. and Bruner, G.H. 1984, Bull. Amer. Astron. Soc., 16, 492.Google Scholar