Physical properties of central stars of planetary nebulae

Details Physical properties of central stars of planetary nebulae Physical properties of central stars of planetary nebulae

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281b.169p&link_type=abstract

In ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2 p 169-172 (SEE N89

Astronomy and Astrophysics

Astronomy

1

Iue, Planetary Nebulae, Spaceborne Astronomy, Stellar Spectra, Ultraviolet Astronomy, Ultraviolet Spectra, Stellar Atmospheres, Stellar Color, Stellar Models

Scientific paper

The UV spectra of central stars of planetary nebulae (PNCS), obtained with the IUE, were used to investigate the fundamental stellar parameters of these stars. All the low resolution data of PNCS observed before Jan. 1, 1984 were examined. From non-LTE model atmospheres information on the color temperature in the UV range for those PNCS observed with a relatively good signal-to-noise ratio in the short and in the long wavelength range of IUE is obtained.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1180874