The ionization structure of planetary nebulae. IX - NGC 1535

Details The ionization structure of planetary nebulae. IX - NGC 1535 The ionization structure of planetary nebulae. IX - NGC 1535

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...340..921b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 340, May 15, 1989, p. 921-926.

Astronomy and Astrophysics

Astrophysics

11

Ionization, Planetary Nebulae, Spectrophotometry, Ultraviolet Spectra, Abundance, Balmer Series, Electron Energy, Emission Spectra, Interstellar Extinction

Scientific paper

The ionization structure of planetary nebula NGC 1535 was investigated using spectrophotometric observations of emission-line intensities over the spectral range 1400-7200 A, which were carried out in five positions in this nebula. The results obtained on the ionic abundances of He, O, N, Ne, C, and Ar in NGC 1535 suggest that it is a planetary nebula that formed initially in a somewhat metal-poor region and has undergone little or no enhancement of its original abundances by mixing with nuclear-processed material.

Affiliated with

Also associated with

No associations

Rating

The ionization structure of planetary nebulae. IX - NGC 1535 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 The ionization structure of planetary nebulae. IX - NGC 1535, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The ionization structure of planetary nebulae. IX - NGC 1535 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1874178