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Distribution de l'énergie dans le spectre ultraviolet de quelques étoiles

  • D. Chalonge (a1), L. Divan (a1) and C. T. Hua (a2)

Abstract

Preliminary results of recent direct comparisons between some early type O, B standards (and also α Lyr) and a terrestrial source previously compared to a black body are given for the ultraviolet range. It appears that the previously-used gradients ɸuv must be corrected on the average by +0.10.

Résumé

On donne les résultats préliminaires des comparaisons directes entre quelques étoiles, O, B (et également de α Lyr) et une source terrestre préalablement rapportée au corps noir. Il semble que les gradients ultraviolets utilisés jusqu'ici doivent être corrigés de +0,10 en moyenne.

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Copyright

References

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Baillet, A. et Chalonge, D.: 1973, Nouvelle Revue d'Optique Appliquée , à paraître.
Barbier, D. et Chalonge, D.: 1941, Ann. Astrophys. 4, 30.
Chalonge, D. et Servigne, M.: 1952, Ann. Astrophys. 15, 151.
Chalonge, D. et Divan, L.: 1972, à paraître.
Chalonge, D. et Hua, C. T.: 1972, à paraître.
Divan, L.: 1966, Lodén, dans K., Lodén, L. O., and Sinnerstad, U. (eds.), ‘Spectral Classification and Multicolour Photometry’, IAU Symp. 24, 311.

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