Abstract
The UV energy curve of Canopus in the 2400–4000 Å wavelength range has been obtained from spectrograms having a dispersion of 183 Å mm-1. This curve is in good agreement with previous observations and with a model atmosphere. The equivalent width of MgII 2795 Å, 2802 Å is found to be 22 Å.
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Kondo, Y., Henize, K.G., Kotila, C.L. (1970). UV Spectrophotometry of Canopus from Gemini XI. In: Houziaux, L., Butler, H.E. (eds) Ultraviolet Stellar Spectra and Related Ground-Based Observations. International Astronomical Union / Union Astronomique Internationale, vol 36. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3293-3_31
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DOI: https://doi.org/10.1007/978-94-010-3293-3_31
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3295-7
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