Internal motions of fourteen planetary nebulae

Details Internal motions of fourteen planetary nebulae Internal motions of fourteen planetary nebulae

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...136..200s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 136, no. 2, July 1984, p. 200-205. Research supported by the Consiglio Naziona

Astronomy and Astrophysics

Astrophysics

16

Astronomical Spectroscopy, H Beta Line, Planetary Nebulae, Stellar Motions, Astronomical Models, Gas Dynamics, Spectral Line Width, Stellar Evolution

Scientific paper

High dispersion spectra allowed the authors to obtain the expansion velocity, Hβ flux and angular dimension of fourteen planetary nebulae. All the nebulae of this sample are in a rather early evolutionary phase (nebular radius <0.07 pc) and present expansion velocities smaller than 15 km s-1. The observational parameters, i.e. nebular radius, expansion velocity, nebular mass, temperature, radius and luminosity of the central star (for two objects) can be explained in terms of the "two-phase" evolutionary model suggested by Sabbadin et al. (1984).

Affiliated with

Also associated with

No associations

Rating

Internal motions of fourteen 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 Internal motions of fourteen planetary nebulae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Internal motions of fourteen planetary nebulae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1703991