Skip to main content

Energetic Outflows from Young Stars

The radiation emitted by carbon monoxide molecules in clouds of gas and dust where new stars are forming discloses masses of gas moving outward at high velocity in opposed directions

00
Scientific American Magazine Vol 247 Issue 1This article was originally published with the title “Energetic Outflows from Young Stars” in Scientific American Magazine Vol. 247 No. 1 (), p. 82
doi:10.1038/scientificamerican0782-82