FUSE Time Resolved Spectroscopy of the LMC O9.7 Ib Star HD 268605

Details FUSE Time Resolved Spectroscopy of the LMC O9.7 Ib Star HD 268605 FUSE Time Resolved Spectroscopy of the LMC O9.7 Ib Star HD 268605

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...195.0625m&link_type=abstract

American Astronomical Society, 195th AAS Meeting, #06.25; Bulletin of the American Astronomical Society, Vol. 31, p.1378

Astronomy and Astrophysics

Astronomy

Scientific paper

We present spectra covering the wavelength range 990 < λ < 1190 Angstroms for the LMC O9.7 Ib star HD 268605 (= Sk -67 005). The observations illustrate the high quality of data currently available from FUSE. They also demonstrate the capabilities of FUSE to provide time resolved spectroscopy of wind and photospheric lines never before explored for temporal variability in a systematic manner. The observations span several days, with one continuously sampled interval of more than 4 hours. The mean spectrum also serves as an excellent example of the dense information content of the FUSE spectral region. It contains a wealth of both stellar and interstellar lines which cover a wide range of ionization and, hence, physical conditions. This work is supported by NASA contract NAS5-32985.

Affiliated with

Also associated with

No associations

Rating

FUSE Time Resolved Spectroscopy of the LMC O9.7 Ib Star HD 268605 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 Time Resolved Spectroscopy of the LMC O9.7 Ib Star HD 268605, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and FUSE Time Resolved Spectroscopy of the LMC O9.7 Ib Star HD 268605 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1735754