Computer Science
Scientific paper
May 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1135..154i&link_type=abstract
FUTURE DIRECTIONS IN ULTRAVIOLET SPECTROSCOPY: A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic
Computer Science
Binary And Multiple Stars, Photometric, Polarimetric, And Spectroscopic Instrumentation, General, Solar Nebula, Cosmogony
Scientific paper
We present FUV observations of massive binary systems in the Galaxy, LMC and SMC. The binaries are High Mass X-ray binaries and double-line spectroscopic binaries. Many are eclipsing systems, with well-determined orbits and periods in the range 1.6-12 days. The far-UV spectra are used to determine spectrometric changes with phase and terminal velocities from species tracing a range of wind ionization states. We observed each system more than once to sample different orbital phases and spectral variability. All systems show significant changes in the P-Cygni wind profiles with phase.
Gies Doug
Iping Rosina C.
Sonneborn George
Williams Steve
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