Consequences of the Solar System passage through dense interstellar clouds
Several consequences of the passage of the solar system through dense interstellar molecular clouds are discussed. These clouds, dense (more than 100 cm<sup>-3</sup>), cold (10–50 K) and extended (larger than 1 pc), are characterized by a gas-to-dust mass ratio of about 100, by a...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2003-06-01
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| Series: | Annales Geophysicae |
| Online Access: | https://www.ann-geophys.net/21/1263/2003/angeo-21-1263-2003.pdf |