Astronomy Letters

, Volume 32, Issue 9, pp 604–607

Spectrophotometric observations of variable stars

Authors

  • E. V. Ruban
    • Pulkovo Astronomical ObservatoryRussian Academy of Sciences
  • G. A. Alekseeva
    • Pulkovo Astronomical ObservatoryRussian Academy of Sciences
  • A. A. Arkharov
    • Pulkovo Astronomical ObservatoryRussian Academy of Sciences
  • E. I. Hagen-Thorn
    • Pulkovo Astronomical ObservatoryRussian Academy of Sciences
  • V. D. Galkin
    • Pulkovo Astronomical ObservatoryRussian Academy of Sciences
  • I. N. Nikanorova
    • Pulkovo Astronomical ObservatoryRussian Academy of Sciences
  • V. V. Novikov
    • Pulkovo Astronomical ObservatoryRussian Academy of Sciences
  • V. P. Pakhomov
    • Pulkovo Astronomical ObservatoryRussian Academy of Sciences
  • T. Yu. Puzakova
    • Pulkovo Astronomical ObservatoryRussian Academy of Sciences
Article

DOI: 10.1134/S1063773706090052

Cite this article as:
Ruban, E.V., Alekseeva, G.A., Arkharov, A.A. et al. Astron. Lett. (2006) 32: 604. doi:10.1134/S1063773706090052

Abstract

We present the results of our visual and near-infrared spectrophotometric observations for 77 variable stars obtained during 1971–1991 in Chile, Armenia, and Bolivia. The quasi-monochromatic, extraatmospheric fluxes from the stars are given in absolute energy units (W m−2 m−1) at all wavelengths of the spectral range at 2.5-nm intervals.

PACS numbers

95.80.+p95.85.Kr95.85.Jq95.85.Ls

Key words

stars—variable and peculiarspectrophotometric catalogsspectrophotometry

Copyright information

© Pleiades Publishing, Inc. 2006