An HST COS SNAPshot Spectrum of the K Supergiant l Vel (K4Ib-II)
Buried Alive in the Coronal Graveyard
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
Physical structure of the local interstellar medium
Space Telescope Imaging Spectrograph Survey of Far-Ultraviolet Coronal Forbidden Lines in Late-Type Stars
Stellar population astrophysics (SPA) with the TNG. The Arcturus Lab
The Amazing COS FUV (1320 - 1460 A) Spectrum of l Vel (K4Ib-II)1
The interstellar cloud surrounding the Sun: a new perspective
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 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 Wind Temperature and Mass-loss Rate of Arcturus (K1.5 III)
UV and EUV observations of stellar coronal structure and activity
Instrument
STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
1998-08-24T17:11:46Z/1998-08-24T22:45:18Z
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, Ayres comma Thomas R., 1999, 'Distant Futures of Solar Activity', 1.0, European Space Agency, https://doi.org/10.5270/esa-xy4v9j7