Investigating the kinematics of the faint, giant haloes of Planetary Nebulae

Details Investigating the kinematics of the faint, giant haloes of Planetary Nebulae Investigating the kinematics of the faint, giant haloes of Planetary Nebulae

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.216...23b&link_type=abstract

Astrophysics and Space Science, vol. 216, no. 1-2, p. 23-24

Astronomy and Astrophysics

Astrophysics

Kinematics, Planetary Nebulae, Stellar Envelopes, Stellar Evolution, Stellar Spectra, Astronomical Spectroscopy, Emission Spectra, Line Spectra, Stellar Models

Scientific paper

Some interesting results from a current program of high resolution spectroscopy of the faint, giant haloes of Planetary Nebulae are presented. Observations of optical emission line profiles show that these haloes have very little turbulent motion. The halo of NGC 6543 is thought to be a filamentary, thin, radially expanding, spherical shell and that of NGC 6826 is more probably a filled spherical shell. The halo of NGC 6720 contains inner and outer shells, the split profiles from the inner halo show that this part of the halo is bipolar in nature.

Affiliated with

Also associated with

No associations

Rating

Investigating the kinematics of the faint, giant haloes of 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 Investigating the kinematics of the faint, giant haloes of Planetary Nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Investigating the kinematics of the faint, giant haloes of Planetary Nebulae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1862550