Hostname: page-component-745bb68f8f-b95js Total loading time: 0 Render date: 2025-01-13T00:12:49.036Z Has data issue: false hasContentIssue false
  • English
  • Français

A new fuor?

Published online by Cambridge University Press:  23 September 2016

H.M. Tovmassian ,
R.Kh. Hovhannessian  and
R.A. Epremian
H.M. Tovmassian
Affiliation:
Byurakan Astrophysical Observatory Armenian Academy of Sciences, USSR
R.Kh. Hovhannessian
Affiliation:
Byurakan Astrophysical Observatory Armenian Academy of Sciences, USSR
R.A. Epremian
Affiliation:
Byurakan Astrophysical Observatory Armenian Academy of Sciences, USSR

Extract

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.

During observations made in August and November 1987 with the ultraviolet telescope “Glasar” [1] installed at the module “Kwant” of the “Mir” Space Station a very blue star HD 269665 = Sk −68°110 in the region of the LMC was detected.

Type
III Flare Stars and Related Objects Fuors and Other Non-Stable Objects
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 261 - 262
Copyright
Copyright © Kluwer 1990 

References

1. Tovmassian, H. M., Khodjayantz, Yu.M., Krmoyan, M.N., Kashin, A.L., Zakharian, A.Z., Hovhanessian, R.Kh., Mkrtchian, M.A., Tovmassian, G.H. Huguenin, D., Bootov, V.V., Romanenko, Yu. V., Laveikin, A.J. and Alexandrov, A.P. (1988), ‘“Glazar” - the orbital ultraviolet telescope’, Pisma v A.J., 14, 291–295.Google Scholar
2. Shobbrook, R.R., and Visvanathan, N. (1987), ‘The distance to the LMC from uvbyβ photometry of B stars’ Monthly Notices Roy. Astron, Soc., 225, 947–960.Google Scholar
3. Sanduleak, N. (1969) ‘A deep objective - prism survey for LMC member’, Cerro-Tololo Interamerican Observatory, Contr. No.89.Google Scholar
4. Thompson, G.J., Nandy, K., Jamar, C., Monfiles, A., Houziaux, L., Carnochan, D.J. and Wilson, R. (1978) ‘Catalogue of stellar ultraviolet fluxes’, The Science Research Council pp. 1–449.Google Scholar