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- W1675821657 abstract "We present a list of interstellar absorption lines in the direction of HD 37061 in the M 43 nebula. Some of the absorption lines arise from atomic excited levels that are uncommon in interstellar clouds. The excited levels of Fe II are populated by fluorescence. We found a large number of H2 molecular absorption lines arising from vibrationally excited levels. The ortho/para H2 ratio is equal to 2.7. The H2 rotational temperature of vibrational levels 1 - 5 exceeds 2000 K." @default.
- W1675821657 created "2016-06-24" @default.
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- W1675821657 date "2008-12-31" @default.
- W1675821657 modified "2023-10-17" @default.
- W1675821657 title "Interstellar medium in the M 43 nebula" @default.
- W1675821657 hasPublicationYear "2008" @default.
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