Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...482l..97b&link_type=abstract
Astrophysical Journal Letters v.482, p.L97
Astronomy and Astrophysics
Astronomy
64
Ism: Planetary Nebulae: Individual Alphanumeric: He 3-, 475, Ism: Jets And Outflows, Hydrodynamics, Shock Waves
Scientific paper
The proto--planetary nebula He 3-1475 was imaged in the [N II] lambda 6584 line with the Wide Field Planetary Camera 2 on board the Hubble Space Telescope. This image has revealed what appear to be large-scale flows being collimated into narrow bipolar jets. This is a unique object: we may be observing the actual collimation process of an astrophysical jet. Analytical models and hydrodynamical simulations suggest that the jet in He 3-1475 may be produced by purely hydrodynamical means, through focusing of a weakly collimated bipolar outflow into jets by oblique radiative shocks.
Blondin John M.
Borkowski Kazimierz J.
Harrington Patrick J.
No associations
LandOfFree
Collimation of Astrophysical Jets: The Proto-Planetary Nebula He 3-1475 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Collimation of Astrophysical Jets: The Proto-Planetary Nebula He 3-1475, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Collimation of Astrophysical Jets: The Proto-Planetary Nebula He 3-1475 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1473008