Characterizing the Stellar Population in NGC 1705-1
Cold diffuse interstellar medium of Magellanic Clouds: II. Physical conditions from excitation of C I and H2
Interstellar Gas-phase Element Depletions in the Small Magellanic Cloud: A Guide to Correcting for Dust in QSO Absorption Line Systems
Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
On the weak Lya emission line of BL Lacertae objects
Optically thick structure in early B-type supergiant stellar winds at low metallicities
Optimization of Starburst99 for Intermediate-Age and Old Stellar Populations
StarCAT: A Catalog of Space Telescope Imaging Spectrograph Ultraviolet Echelle Spectra of Stars
Terminal Velocities of Luminous, Early-Type Stars in the Small Magellanic Cloud
The Ultraviolet and Optical Spectra of Luminous B-Type Stars in the Small Magellanic Cloud
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, STIS/NUV-MAMA
Temporal Coverage
2001-10-16T00:30:05Z/2003-03-20T09:19:49Z
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., 2006, 'Understanding high-redshift and starburst galaxies: A UV spectroscopic survey of B- stars in the SMC', 1.0, European Space Agency, https://doi.org/10.5270/esa-tpqr8wd