665 citations · 1.7k across the 7 of their papers we have counts for
7 papers
The Cosmic Origins Spectrograph
James C. Green, Cynthia S. Froning, Steve Osterman +23
The Cosmic Origins Spectrograph (COS) is a moderate-resolution spectrograph with unprecedented sensitivity that was installed into the Hubble Space Telescope (HST) in May 2009, dur…
Optical Structure and Proper-Motion Age of the Oxygen-rich Supernova Remnant 1E 0102-7219 in the Small Magellanic Cloud
Steven L. Finkelstein, Jon A. Morse, James C. Green +12
We present new optical emission-line images of the young SNR 1E 0102-7219 (E0102) in the SMC obtained with the HST Advanced Camera for Surveys (ACS). E0102 is a member of the oxyge…
On-Orbit Performance of the Far Ultraviolet Spectroscopic Explorer (FUSE) Satellite
D. J. Sahnow, H. W. Moos, T. Ake +38
Launch of the Far Ultraviolet Spectroscopic Explorer (FUSE) has been followed by an extensive period of calibration and characterization as part of the preparation for normal satel…
Overview of the Far Ultraviolet Spectroscopic Explorer Mission
H. W. Moos
The Far Ultraviolet Spectroscopic Explorer satellite observes light in the far-ultraviolet spectral region, 905 - 1187 A with high spectral resolution. The instrument consists of f…
The Detection of Wind Variability in Magellanic Cloud O Stars
D. Massa, A. W. Fullerton, J. B. Hutchings +8
We present Far Ultraviolet Explorer (FUSE) spectra for three Magellanic Cloud O stars (Sk 80, Sk -67 05 and Sk -67 111) with repeated observations. The data demonstrate the capabil…
Far-UV FUSE spectroscopy of the OVI resonance doublet in Sand2 (WO)
Paul A. Crowther, A. W. Fullerton, D. J. Hillier +10
We present Far-Ultraviolet Spectroscopic Explorer (FUSE) spectroscopy of Sand 2, a LMC WO-type Wolf-Rayet star, revealing the OVI resonance P Cygni doublet at 1032-38A. These data…
FUSE Observations of the Stellar Winds of Two O7 Supergiants in the Magellanic Clouds
A. W. Fullerton, P. A. Crowther, O. De Marco +10
We compare the stellar wind features in far-UV spectra of Sk -67 111, an O7 Ib(f) star in the LMC, with Sk 80, an O7 Iaf+ star in the SMC. The most striking differences are that Sk…