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- W125636342 abstract "The first results of detailed spectroscopy are presented for carbon Mira R Leporis. This long-period variable is undergoing deep fadings, apparently caused by dust formation around the star. High-resolution CCD spectra were observed for two seasons. The heliocentric photospheric radial velocity was found to be +32.6 and +38.4 km s -1 , respectively. Blueshifted emissions from the circumstellar gas are seen." @default.
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- W125636342 date "2005-01-01" @default.
- W125636342 modified "2023-10-09" @default.
- W125636342 title "THE SPECTROSCOPY OF THE PULSATING CARBON STAR R Lep" @default.
- W125636342 doi "https://doi.org/10.18524/1810-4215.2005.18.98274" @default.
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