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• W4385948929 abstract "The IR spectra of Be stars display numerous hydrogen recombination lines, constituting a great resource for obtaining information on the physical and dynamic structures of different regions within the circumstellar envelope. Nevertheless, this spectral region has not been analysed in depth, and there is a lack of synthetic spectra with which to compare observations. Therefore, we computed synthetic spectra with the HDUST code for different disc parameters. Here, we present our results on the spectral region that includes lines of the Brackett series. We discuss the dependence of the line series strengths on several parameters that describe the structure of the disc. We also compared model line profiles, fluxes, and EWs with observational data for two Be stars (MX Pup and π Aqr). Even though the synthetic spectra adequately fit our observations of both stars and allow us to constrain the parameters of the disc, there is a discrepancy with the observed data in the EW and flux measurements, especially in the case of MX Pup. It is possible that by including Brackett lines of higher terms or adding the analysis of other series, we may be able to better constrain the parameters of the observed disc." @default.
• W4385948929 created "2023-08-18" @default.
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• W4385948929 date "2023-08-17" @default.
• W4385948929 modified "2023-10-16" @default.
• W4385948929 title "Infrared Spectroscopy of Be Stars: Influence of the Envelope Parameters on Brackett-Series Behaviour" @default.
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• W4385948929 doi "https://doi.org/10.3390/galaxies11040090" @default.
• W4385948929 hasPublicationYear "2023" @default.
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