A ~ 40 Year Variability Cycle in the Luminous Blue Variable/Wolf-Rayet Binary System HD 5980?
A Far Ultraviolet Spectroscopic Explorer Survey of Interstellar O VI Absorption in the Small Magellanic Cloud
A Tale of Two Stars: The Extreme O7 Iaf+ Supergiant AV 83 and the OC7.5 III((f)) star AV 69
Cold diffuse interstellar medium of Magellanic Clouds: II. Physical conditions from excitation of C I and H2
Effects of Metallicity on the Rotational Velocities of Massive Stars
Fundamental Properties of O-Type Stars
Hubble Space Telescope Observations of the Luminous Blue Variable/W-R Eclipsing Binary System HD 5980
Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
Massive stars at low metallicity. Evolution and surface abundances of O dwarfs in the SMC
Massive stars in the Small Magellanic Cloud. Evolution, rotation, and surface abundances
NLTE Line-Blanketed Model Stellar Atmospheres
No breakdown of the radiatively driven wind theory in low-metallicity environments
Optically thick structure in early B-type supergiant stellar winds at low metallicities
Quantitative Spectroscopy of O Stars at Low Metallicity: O Dwarfs in NGC 346
StarCAT: A Catalog of Space Telescope Imaging Spectrograph Ultraviolet Echelle Spectra of Stars
STIS Spectral Imagery of the OB Stars in NGC 604. I. Description of the Extraction Technique for a Crowded Stellar Field
Terminal Velocities of Luminous, Early-Type Stars in the Small Magellanic Cloud
The Confusion Limit on Astrometry with the Space Interferometry Mission
The Photospheric Absorption Lines in the Ultraviolet Spectrum of the Multiple System HD 5980
The Ultraviolet and Optical Spectra of Luminous B-Type Stars in the Small Magellanic Cloud
The Ultraviolet and Optical Spectra of Metal-deficient O Stars in the Small Magellanic Cloud
Tiny-scale molecular structures in the Magellanic Clouds. I. FUSE, HST and VLT observations
Ultraviolet Line Spectra of Metal-poor Star-forming Galaxies
Using Shell models to investigate clumping in the wind of the O7Iaf + supergiant AzV83
UV Spectroscopy of Metal-Poor Massive Stars in the Small Magellanic Cloud
Winds of Low-metallicity OB-type Stars: HST-COS Spectroscopy in IC 1613
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
1998-08-08T00:16:26Z/2000-11-23T01:11:51Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Lennon comma Daniel J., 2000, 'Understanding high-redshift and starburst galaxies: A UV spectroscopic survey of O-stars in the SMC', 1.0, European Space Agency, https://doi.org/10.5270/esa-nqa8p09