The interaction of the eta carinae primary wind with a century old slow equatorial ejecta
We argue that the asymmetric morphology of the blue and red shifted components of the
outflow at hundreds of AU from the massive binary system η Carinae can be understood …
outflow at hundreds of AU from the massive binary system η Carinae can be understood …
Physics of the Inner Ejecta
F Hamann - Eta Carinae and the Supernova Impostors, 2012 - Springer
Eta Carinae's inner ejecta are dominated observationally by the bright Weigelt blobs and
their famously rich spectra of nebular emission and absorption lines. They are dense (ne∼ …
their famously rich spectra of nebular emission and absorption lines. They are dense (ne∼ …
Eta Carinae--Physics of the Inner Ejecta
F Hamann - arXiv preprint arXiv:1212.3348, 2012 - arxiv.org
Eta Carinae's inner ejecta are dominated observationally by the bright Weigelt blobs and
their famously rich spectra of nebular emission and absorption lines. They are dense (n_e …
their famously rich spectra of nebular emission and absorption lines. They are dense (n_e …
Spectroscopy and Interferometry of the Winds of Luminous Blue Variables
ND Richardson - 2012 - scholarworks.gsu.edu
Massive stars are rare, but emit most of the light we observe in the Universe and create
many of the heavy elements. New observational approaches and long time-series are …
many of the heavy elements. New observational approaches and long time-series are …
The Winds of Eta Carinae and Other Very Luminous Stars
FP Najarro, DJ Hillier - Eta Carinae and the Supernova Impostors, 2012 - Springer
Abstract The winds of Eta Carinae, other related very luminous stars, and candidate LBVs
are reviewed. While ground-based spectra of η Car are influenced by multiple emission …
are reviewed. While ground-based spectra of η Car are influenced by multiple emission …