Goddard High-Resolution Spectrograph Observations of Cool Low-Gravity Stars. IV. A Comparison of the K5 III stars a Tauri and g Draconis
Hubble Space Telescope Constraints on the Winds and Astrospheres of Red Giant Stars
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
OI line emission in cool stars: calculations using partial redistribution
On Chromospheric Heating Mechanisms of ``Basal Flux Stars
Physical structure of the local interstellar medium
The interstellar cloud surrounding the Sun: a new perspective
The outer atmosphere of Tau - I. A new chromospheric model
The outer atmosphere of Tau - II. Fluorescent lines
The outer atmosphere of a Tau - III. Inhomogeneities deduced from cold CO fluorescence
The Structure of the Local Interstellar Medium. I. High-Resolution Observations of Fe II, Mg II, and Ca II toward Stars within 100 Parsecs
The Structure of the Local Interstellar Medium. III. Temperature and Turbulence
The three-dimensional physical structure of the local interstellar medium
The Wind-ISM Interaction of a Tauri
Instrument
HRS, HRS/2
Temporal Coverage
1994-04-07T22:25:17Z/1994-04-08T12:58:12Z
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., 1995, 'THE CHROMOSPHERE OF ALPHA TAU - CYCLE 4 MEDIUM', 1.0, European Space Agency, https://doi.org/10.5270/esa-kwxp44v
