Line widths in peculiar emission line objects

Details Line widths in peculiar emission line objects Line widths in peculiar emission line objects

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...103l...3s&link_type=abstract

Astronomy and Astrophysics, vol. 103, no. 1, Nov. 1981, p. L3, L4.

Astronomy and Astrophysics

Astrophysics

16

Emission Spectra, Interstellar Matter, Line Spectra, Planetary Nebulae, Protoplanets, Spectral Line Width, Binary Stars, Spectrum Analysis, Stellar Evolution

Scientific paper

Emission line profiles of a series of objects such as protoplanetary nebulae, Be stars, symbiotic stars, and young planetary nebulae have been studied to test the interacting wind hypothesis. Measurements of the line widths of H-alpha, He I, and forbidden N II accomplished by television techniques are found to be consistent with the interacting wind hypothesis for the formation of planetary nebulae.

Affiliated with

Also associated with

No associations

Rating

Line widths in peculiar emission line objects 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 Line widths in peculiar emission line objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Line widths in peculiar emission line objects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-743347