Constraints on the Structure of the Heliospheric Interface Based on Ly a Absorption Spectra
CoolCAT
Correlating Intrinsic Stellar Parameters with Mg II Self-reversal Depths
Dependence of Heliospheric Lya Absorption on the Interstellar Magnetic Field
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
Karl Schwarzschild Lecture: What Hyades F Stars tell us about Heating Mechanisms in the outer Stellar Atmospheres (With 15 Figures)
Lya Absorption from Heliosheath Neutrals
Mg II Emission Lines of Hyades F Stars
Mg II h + k Flux--Rotational Period Correlation for G-type Stars
Microstructure of the Local Interstellar Cloud and the Identification of the Hyades Cloud
Stellar Lya Emission Lines in the Hubble Space Telescope Archive: Intrinsic Line Fluxes and Absorption from the Heliosphere and Astrospheres
The O VI and C III Lines at 1032 and 977 A in Hyades F Stars
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
What Is Happening at Spectral Type F5 in Hyades F Stars?
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
1998-10-26T17:24:58Z/1999-08-03T17:39:14Z
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, Boehm-Vitense comma Erika, 2006, 'Chromospheres and transition layers in Hyades and Pleiades F stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-yjkzzfe