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- W565533268 abstract "AbstractThe Herschel Gould Belt Survey far-IR maps of the Orion L 1641 molecular clouds have revealed a wealth of interconnected filaments and dense sources in the region. We report here the first estimation of the total mass of the L 1641 clouds as derived from dust (3. 7 × 104 M⊙). We further present our initial analysis of the physical properties of these dense sources as a result of their immediate environment. We have extracted a robust and statistically significant sample of 321 pre-stellar sources with a mass distribution that spans a range of 0.1–20 M⊙. We show that there are two mass range distributions that depend on the location of the dense cores on or off the identified filaments.KeywordsSpectral Energy DistributionFilamentary StructureDense SourceInitial Mass FunctionEmissivity IndexThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves." @default.
- W565533268 created "2016-06-24" @default.
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- W565533268 date "2014-01-01" @default.
- W565533268 modified "2023-09-23" @default.
- W565533268 title "Filaments and Pre-stellar Sources in the Orion A L 1641 Molecular Clouds" @default.
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- W565533268 doi "https://doi.org/10.1007/978-3-319-03041-8_48" @default.
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