A Multiwavelength Campaign on g Cassiopeiae. III. The Case for Magnetically Controlled Circumstellar Kinematics
A Multiwavelength Campaign on g Cassiopeiae. II. The Case for Corotating, Circumstellar Clouds
A Multiwavelength Campaign on g Cassiopeiae. I. The Case for Surface X-Ray Flaring
A Multiwavelength Campaign on g Cassiopeiae. IV. The Case for Illuminated Disk-enhanced Wind Streams
Automated Photometry of g Cassiopeiae: The Last Roundup
Short-term variability and mass loss in Be stars. V. Space photometry and ground-based spectroscopy of g Cas
The X-ray emission of the g Cassiopeiae stars
Ultraviolet Activity as Indicators of Small-scale Magnetic Fields in g Cassiopeiae
Instrument
HRS, HRS/2
Temporal Coverage
1996-03-14T20:04:04Z/1996-03-15T18:56:38Z
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, Smith comma Myron A., 1997, 'SEARCHING FOR FLARING ACTIVITY ON THE BE STAR GAMMA CAS', 1.0, European Space Agency, https://doi.org/10.5270/esa-2pb3ucn