Far UV excess and gas content of SO galaxies

Details Far UV excess and gas content of SO galaxies Far UV excess and gas content of SO galaxies

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218...69r&link_type=abstract

In ESA Fourth European IUE Conf. p 69-72 (SEE N84-35135 24-88)

Computer Science

4

Early Stars, Far Ultraviolet Radiation, Galactic Radiation, Iue, Interstellar Gas, Spectrum Analysis, Ultraviolet Spectra

Scientific paper

Preliminary results about the analysis of IUE spectra of S0 galaxies in terms of far-UV excess are given. For the two S0 galaxies considered: NGC 5102 (gas-rich) and NGC 3115 (gas poor), a comparison with optical as well as UV stellar continua gives a uniform stellar population respectively A3 and G2. The UV excesses, normalized to the V band, represent a very low fraction (1 - 2%) of the total emitted energy.

Affiliated with

Also associated with

No associations

Rating

Far UV excess and gas content of SO galaxies 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 Far UV excess and gas content of SO galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Far UV excess and gas content of SO galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1705540