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• W2145558264 abstract "Context. Infrared (IR) spectra provide a prime tool to study the characteristics of polycyclic aromatic hydrocarbon (PAH) molecules in regions of star formation. Herbig Ae/Be stars are a class of young pre-main sequence stellar objects of intermediate mass. They are known to have varying amounts of natal cloud material still present in their direct vicinity." @default.
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• W2145558264 date "2008-04-08" @default.
• W2145558264 modified "2023-10-03" @default.
• W2145558264 title "The characteristics of the IR emission features in the spectra of Herbig Ae stars: evidence for chemical evolution" @default.
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• W2145558264 doi "https://doi.org/10.1051/0004-6361:20078001" @default.
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