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Twisted magnetic field around newborn star confirms decades-old jet theory

Twisted magnetic field around newborn star confirms decades-old jet theory
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Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA), of which the U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) is a partner, have captured the first direct, high-resolution images of a magnetic field wrapped tightly around the outflow of gas streaming away from a forming star—evidence that solves a decades-old puzzle about how young stars sculpt the powerful jets that form them.

Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA), of which the U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) is a partner, have captured the first direct, high-resolution images of a magnetic field wrapped tightly around the outflow of gas streaming away from a forming star—evidence that solves a decades-old puzzle about how young stars sculpt the powerful jets that form them.
the U.S. National Science Foundation National Radio Astronomy Observatory (ORG) NSF (ORG)
Originally published by Phys.org Read original →