Flows in Clumpy Planetary Nebulae

Details Flows in Clumpy Planetary Nebulae Flows in Clumpy Planetary Nebulae

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.245..263h&link_type=abstract

Astrophysics and Space Science, Volume 245, Issue 2, pp.263-273

Astronomy and Astrophysics

Astrophysics

5

Planetary Nebulae, Hydrodynamics, Multi-Phase Flows

Scientific paper

The dynamics of clumps observed in planetary nebulae are considered. The possibility that SiO maser spots in evolved stars and the planetary nebula clumps are formed by the Parker instability behind shocks in pulsating stars' atmospheres is raised. Molecular observations of the clumps are suggested. The effects of the ablation of clumps on the global flow structure of a more tenuous plasma in which they are embedded are reviewed.

Affiliated with

Also associated with

No associations

Rating

Flows in Clumpy Planetary Nebulae 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 Flows in Clumpy Planetary Nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Flows in Clumpy Planetary Nebulae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1458525