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- W3100828258 abstract "We present the optical spectroscopic study based on 41 spectra of 4 Her and 32 spectra of 88 Her, obtained over a period of 6 months. We estimate the rotational velocity of these stars from He{sc i} lines in the blue spectral region (4000--4500 AA). We find that these stars are likely to be rotating at a fractional critical rotation of $sim$ 0.80. We measure the average $I_p/I_c$ ratio to quantify the strength of the H$alpha$ line and obtain 1.63 for 4 Her and 2.06 for 88 Her. The radius of the H$alpha$ emission region is estimated to be $R_d/R_*$ $sim$ 5.0, assuming a Keplerian disk. These stars are thus found to be fast rotators with relatively small H$alpha$ emission region. We detect V/R variation of H$alpha$ spectral line during the observed period. We re-estimate the periods for both the stars and obtain two periods of $sim$ 46 days and its harmonic of 23.095 days for 4 Her and $sim$ 86 days for 88 Her. As these two are shell stars with binaries and have low H$alpha$ EW with the emission region closer to the central star, the V/R variation and a change in period may be an effect of the binary on the circumstellar disk." @default.
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- W3100828258 date "2016-04-29" @default.
- W3100828258 modified "2023-10-18" @default.
- W3100828258 title "Spectroscopic study of Be-shell stars: 4 Her and 88 Her" @default.
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- W3100828258 doi "https://doi.org/10.1088/1674-4527/16/5/076" @default.
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