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- W1913002015 abstract "ISO has provided us with a new perspective on gas temperatures in photodissociation regions through measurements of line emission from rotationally-excited levels of the H_2 molecule. The H_2 rotational level populations provide a thermal probe, showing that gas temperatures T_gas approx 500-1000 K prevail in a portion of the PDR where significant quantities of H_2 are present. Such high gas temperatures were unexpected. Theoretical models for the S140 PDR are presented. Possible mechanisms for heating the gas to such high temperatures are discussed." @default.
- W1913002015 created "2016-06-24" @default.
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- W1913002015 date "1999-02-26" @default.
- W1913002015 modified "2023-09-27" @default.
- W1913002015 title "Heating the Gas in Photodissociation Fronts" @default.
- W1913002015 doi "https://doi.org/10.48550/arxiv.astro-ph/9902379" @default.
- W1913002015 hasPublicationYear "1999" @default.
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