A collimated jet of molecular gas from a star on the asymptotic giant branch.
Evolved stars of about one solar mass are in general spherically symmetric, yet the planetary nebulae that they produce in the next phase of their evolution tend not to exhibit such symmetry. Collimated 'jets' and outflows of material have been observed up to approximately 0.3 parsec from the central stars of planetary nebulae, and precession of those jets has been proposed to explain the observed asymmetries. Moreover, it has recently been shown theoretically that magnetic fields could launch and collimate such jets. Here we report the detection of a collimated and precessing jet of molecular gas that is traced by water-vapour maser spots approximately 500 astronomical units (au) from the star W43A in Aquila. We conclude that the jet is formed in the immediate vicinity of the star, and infer that elongated planetary nebulae are formed by jets during the short period, of less than 1,000 years, when the star makes its transition through the proto-planetary nebula phase to become a planetary nebula.
Imai
Hiroshi
H
VERA Project Office, National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan. imai@jive.nl
Obara
Kumiko
K
Diamond
Philip J
PJ
Omodaka
Toshihiro
T
Sasao
Tetsuo
T