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- W1983869974 abstract "Context. Molecular hydrogen (H2) is the most abundant molecule in the circumstellar (CS) environments of young stars, and is a key element in giant planet formation. The measurement of the H2 content provides the most direct probe of the total amount of CS gas, especially in the inner warm planet-forming regions of the disks." @default.
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- W1983869974 date "2008-08-01" @default.
- W1983869974 modified "2023-09-27" @default.
- W1983869974 title "Searching for molecular hydrogen mid-infrared emission in the circumstellar environments of Herbig Be stars" @default.
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- W1983869974 doi "https://doi.org/10.1051/0004-6361:200809576" @default.
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