FUSE UV spectrum of HR 5223 (Fremat+, 2002)

Details FUSE UV spectrum of HR 5223 (Fremat+, 2002) FUSE UV spectrum of HR 5223 (Fremat+, 2002)

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..33850986f&link_type=abstract

VizieR On-line Data Catalog: J/A+A/385/986. Originally published in: 2002A&A...385..986F

Computer Science

Stars: Emission

Scientific paper

New spectra have been obtained for the pole-on Be star HR 5223 (HD 120991) using the Far Ultraviolet Satellite Explorer (FUSE). We give a complete description of the far-UV spectral range (920 to 1180Å). The spectra are affected by strong blends with interstellar lines and molecular bands that also significantly lower the energy distribution of the star. We produce a synthetic spectrum of the interstellar medium (ISM) to determine the column densities of several elements (H2, H I, N I, O I ...) seen towards HR 5223 and to disentangle the components due to the ISM, the photosphere and/or to the circumstellar envelope. (1 data file).

Affiliated with

Also associated with

No associations

Rating

FUSE UV spectrum of HR 5223 (Fremat+, 2002) 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 FUSE UV spectrum of HR 5223 (Fremat+, 2002), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and FUSE UV spectrum of HR 5223 (Fremat+, 2002) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1589931