A Non-LTE Analysis of the zeta Aurigae B-Type Secondary. I. Determination of the Fundamental Stellar Parameters
NLTE Radiative Transfer in the Extended Atmospheres and Winds of Cool Stars
The Wind Outflow of zeta Aurigae: A Model Revision Using Hubble Space Telescope Spectra
VLA Observations of z Aurigae: Confirmation of the Slow Acceleration Wind Density Structure
Instrument
HRS, HRS/2
Temporal Coverage
1992-08-31T22:47:05Z/1993-04-12T05:50:23Z
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, Brown comma Alexander, 1994, 'EMPIRICAL DETERMINATION OF THE WIND VELOCITY AND DENSITY LAWS FOR THE K SUPERGIANT ZETA AURIGAE', 1.0, European Space Agency, https://doi.org/10.5270/esa-guwmr24