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Ultraviolet Spectrometry of Peculiar Stars*

Published online by Cambridge University Press:  12 April 2016

G. B. Baratta ,
A. Cassatella  and
R. Viotti
G. B. Baratta
Affiliation:
Osservatorio Astronomico
A. Cassatella
Affiliation:
ESA Villafranca Satellite Tracking Station, Madrid
R. Viotti
Affiliation:
Osservatorio Astronomico

Extract

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The standard classification criteria, when applied to peculiar objects, such as emission line and shell stars, cannot easily be interpreted in terms of their intrinsic physical characteristics. Observations outside the optical spectral region may provide complementary information on their nature leading to a better spectral classification.

Type
VIII Space Spectroscopy and Future Developments in Classification
Information
International Astronomical Union Colloquium , Volume 47: Spectral Classification of the Future , 1979 , pp. 461 - 464
Copyright
Copyright © Vatican Observatory 1979

Footnotes

+

On leave from Laboratorio di Astrofisica Spaziale, Frascati

*

Based on observations by the International Ultraviolet Explorer collected at the Villafranca Satellite Tracking Station of the European Space Agency, Madrid.

References

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Cucchiaro, A., Jaschek, M. and Jaschek, C. (1978). In An Atlas of Ultraviolet Stellar Spectra, preprint. See also Cucchiaro, et al. this conference.Google Scholar
Jamar, C., Macau-Hercot, D., Monfils, A., Thompson, G.I., Houziaux, L. and Wilson, R. (1976). In Ultraviolet Bright Stars Spectrophotometry Catalogue, ESA Scientific Report SR-27, November.Google Scholar
The, , P.S. and Tjin A Djie, H.R.E. (1978). Astron. Astrophys. 62, 439.Google Scholar