Detection of the Compressed Primary Stellar Wind in e Carinae
Eta Carinae: A Tale of Two Periastron Passages
Eta Carinaes 2014.6 spectroscopic event: Clues to the long-term recovery from its Great Eruption
Exploring and Modeling High-excitation Emission in the Ejecta and the Wind of Eta Carinae
He II l4686 Emission from the Massive Binary System in e Car: Constraints to the Orbital Elements and the Nature of the Periodic Minima
Imaging the Time Evolution of Eta Carinaes Colliding Winds with HST
N II ll5668-5712: A New Class of Spectral Features in Eta Carinae
Onthe changes in the physical properties of the ionized region around the Weigelt structures in e Carinae over the 5.54-yr spectroscopic cycle
The fossil wind structures of Eta Carinae: changes across one 5.54-yr cycle
To v and beyond! The He I absorption variability across the 2014.6 periastron passage of e Carinae
Instrument
STIS/CCD
Temporal Coverage
2009-12-06T13:40:03Z/2010-10-26T05:12:18Z
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, Corcoran et al., 2011, 'Monitoring Dynamical Mass Loss from Eta Car with the HETG', 1.0, European Space Agency, https://doi.org/10.5270/esa-cmv8xkh
