Photometric and spectral observations of 7 stars in the WC and WO sequences were made at the Fesenkov Astrophysical Institute in 2021-2022. These observations served as the basis of estimates of the brightness of the objects in BVRc filters and the absolute fluxes of radiation in the emission lines. Changes in the brightness of WR 121 over the limits of 0m.1-0m.15 were recorded. Changes in the fluxes of emission lines were detected in the spectra of several of the objects, WR 4, WR 5, WR 121, and WR 128.
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Translated from Astrofizika, Vol. 67, No. 1, pp. 13-27. (February 2024)
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Kondratyeva, L.N., Reva, I.V., Denissyuk, E.K. et al. Photometric and Spectral Studies of a Group of Wolf-Rayet Galactic Stars. II. WC and WO Sequences. Astrophysics 67, 9–23 (2024). https://doi.org/10.1007/s10511-024-09812-7
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DOI: https://doi.org/10.1007/s10511-024-09812-7