Analysis of H2 Emission from Mira B in Ultraviolet Spectra from the Hubble Space Telescope
An observational study of dust nucleation in Mira (o Ceti). I. Variable features of AlO and other Al-bearing species
Detection of H2 Emission from Mira B in Ultraviolet Spectra from the Hubble Space Telescope
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
Mira B Rejuvenated
Molecular Hydrogen Emission Lines in Far Ultraviolet Spectroscopic Explorer Observations of Mira B
New variations of Mg II emission lines of Mira AB with HST
Saturns wayward shepherds: the peregrinations of Prometheus and Pandora
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
1999-07-26T00:58:59Z/1999-08-02T22:18:17Z
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, Karovska et al., 2007, 'Binary Interaction in the Mira AB Accreting System', 1.0, European Space Agency, https://doi.org/10.5270/esa-825ik0g