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- W67591875 abstract "An investigation of parameters of a sample of more than two hundred late-type long-period variable stars (LPVs) has been carried out. In more detail were studied 13 giants (Mira Ceti-type variables R Aql, RR Aql, RT Aql, R Leo, U Ori, U Her, R Cas, R Tau, Z Cyg, R Peg, U Aur and semiregular variables RT Vir and RX Boo) and 2 supergiants (S Per, PZ Cas). A considerable fraction of the sample stars (about one third) possess circumstellar maser emission in molecular spectral lines (OH, H 2 0, SiO). Our aim was to elucidate the particularities of photometric characteristics of maser stars, such as period P, amplitude A, light curve asymmetry f = (M-m)/P, and, in prospect, to determine their status in course of their evolution on the asymptotic giant branch. An extensive comparison with non-maser LPVs was made." @default.
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- W67591875 date "1989-01-01" @default.
- W67591875 modified "2023-09-27" @default.
- W67591875 title "Investigation of a Sample of Long-Period Variable Stars Possessing Maser Emission" @default.
- W67591875 doi "https://doi.org/10.1017/s025292110006317x" @default.
- W67591875 hasPublicationYear "1989" @default.
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