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- W3100838626 abstract "We investigate the origin of the near-infrared emission of the Herbig Ae star MWC 758 on sub-astronomical unit (AU) scales using spectrally dispersed low resolution () AMBER/VLTI interferometric observations in the H (1.7 μm) and K (2.2 μm) bands. We find that the K band visibilities and closure phases are consistent with the presence of a dusty disk inner rim located at the dust evaporation distance (0.4 AU) while the bulk of the H band emission arises within 0.1 AU from the central star. Comparing the observational results with theoretical model predictions, we suggest that the H band emission is dominated by an hot gaseous accretion disk." @default.
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- W3100838626 date "2008-04-08" @default.
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- W3100838626 title "Gas and dust in the inner disk of the Herbig Ae star MWC 758" @default.
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- W3100838626 doi "https://doi.org/10.1051/0004-6361:200809641" @default.
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