Evaluating Possible Heating Mechanisms Using the Transition Region Line Profiles of Late-Type Stars
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
Lya Absorption in a Croissant-like Heliosphere
Measured Mass-Loss Rates of Solar-like Stars as a Function of Age and Activity
Mg II h + k Flux--Rotational Period Correlation for G-type Stars
Observational Estimates for the Mass-Loss Rates of a Centauri and Proxima Centauri Using Hubble Space Telescope Lya Spectra
The heliospheric hydrogen wall and astrospheres
The Three-dimensional Structure of the Warm Local Interstellar Medium. II. The Colorado Model of the Local Interstellar Cloud
The Three-dimensional Structure of the Warm Local Interstellar Medium. I. Methodology
The a Centauri line of sight: D/H ratio, physical properties of local interstellar gas, and measurement of heated hydrogen (the hydrogen wall) near the heliopause.
Instrument
HRS, HRS/1, HRS/2
Temporal Coverage
1995-05-01T13:19:24Z/1995-05-05T13:51:08Z
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 et al., 1996, 'LOCAL INTERSTELLAR MEDIUM AND D/H RATIO -- REPEAT ALPHA CEN A AND B -- HOPR 145', 1.0, European Space Agency, https://doi.org/10.5270/esa-luansv4