A Comparison of the Outer Atmosphere of the ``Flat Activity Star t Ceti (G8 V) with the Sun (G2 V) and a Centauri A (G2 V)
CoolCAT
HST/STIS high resolution echelle spectra of a Centauri A (G2 V)
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
Mg II h + k Flux--Rotational Period Correlation for G-type Stars
Modeling Mid-Ultraviolet Spectra. I. Temperatures of Metal-poor Stars
Space Telescope Imaging Spectrograph Survey of Far-Ultraviolet Coronal Forbidden Lines in Late-Type Stars
Stellar Activity in the Broadband Ultraviolet
Stellar population astrophysics (SPA) with the TNG. The Arcturus Lab
The Structure of the Local Interstellar Medium. III. Temperature and Turbulence
The Structure of the Local Interstellar Medium. II. Observations of D I, C II, N I, O I, Al II, and Si II toward Stars within 100 Parsecs
The three-dimensional physical structure of the local interstellar medium
The Ups and Downs of a Centauri
Ultraviolet Spectroscopy of Rapidly Rotating Solar-Mass Stars: Emission-line Redshifts as a Test of the Solar-Stellar Connection
UV and EUV observations of stellar coronal structure and activity
X-Ray and Ultraviolet Spectroscopy of Intermediate-Mass, First Crossing Giants
Instrument
STIS, STIS/FUV-MAMA
Temporal Coverage
1999-02-12T01:55:59Z/1999-04-10T05:09:03Z
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, Linsky comma Jeffrey L., 2000, 'Physical Processes in Stellar Atmospheres: Comparative Analysis of the Sun and Alpha Cen A', 1.0, European Space Agency, https://doi.org/10.5270/esa-ke0tx9e