ALMA and VLA reveal the lukewarm chromospheres of the nearby red supergiants Antares and Betelgeuse
A Spatially Resolved, Semiempirical Model for the Extended Atmosphere of a Orionis (M2 Iab)
GHRS Observations of Cool, Low-Gravity Stars. I. The Far-Ultraviolet Spectrum of alpha Orionis (M2 Iab)
HST/GHRS Observations of Cool, Low-gravity Stars. VI. Mass-loss Rates and Wind Parameters for M Giants
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
MG II H and K Profiles in High-Luminosity, Late-Type Stars
Search for CO Absorption Bands in IUE Far-Ultraviolet Spectra of Cool Stars
The Amazing COS FUV (1320 - 1460 A) Spectrum of l Vel (K4Ib-II)1
The First Year With the Hubble Space Telescope
The Outer Atmospheres of Cool, Low Gravity Stars as Revealed by HST
Instrument
HRS, HRS/1, HRS/2
Temporal Coverage
1991-04-26T18:41:25Z/1991-04-27T04:17:30Z
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, Carpenter comma Kenneth G., 1992, 'WINDS OF COOL LUMINOUS STARS: DENSITIES, TEMPERATURES, GEOMETRIC EXTENTS, AND VELOCITY STRUCTURES -- CYCLE 0', 1.0, European Space Agency, https://doi.org/10.5270/esa-q0d5qmc