Eta Carinae: From 1600 to the Present
RM Humphreys, JC Martin - Eta Carinae and the Supernova Impostors, 2012 - Springer
Eta Carinae: From 1600 to the Present Page 1 Chapter 1 Eta Carinae: From 1600 to the Present
Roberta M. Humphreys and John C. Martin Abstract In this introductory chapter we review η …
Roberta M. Humphreys and John C. Martin Abstract In this introductory chapter we review η …
Constraints on the non-thermal emission from η Carinae's blast wave of 1843
JL Skilton, W Domainko, JA Hinton, DI Jones… - Astronomy & …, 2012 - aanda.org
Non-thermal hard X-ray and high-energy (HE; 1 MeV< E< 100 GeV) γ-ray emission in the
direction of η Carinae has been recently detected using the INTEGRAL, AGILE and Fermi …
direction of η Carinae has been recently detected using the INTEGRAL, AGILE and Fermi …
X-ray Variability and the Secondary Star
MF Corcoran, K Ishibashi - Eta Carinae and the Supernova Impostors, 2012 - Springer
We discuss the history of X-ray observations of the η Car system, concentrating on the
periodic variability discovered in the 1990s. We discuss the interpretation of these variations …
periodic variability discovered in the 1990s. We discuss the interpretation of these variations …
High-Resolution Studies of Eta Carinae's Ejecta and Stellar Wind
G Weigelt, S Kraus - Eta Carinae and the Supernova Impostors, 2012 - Springer
Abstract Hubble Space Telescope observations and interferometric measurements provide
unique insights into the small-scale structure of η Car's circumstellar ejecta and its extreme …
unique insights into the small-scale structure of η Car's circumstellar ejecta and its extreme …
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 …
[PDF][PDF] The Star Formation Newsletter
The early stages of the pre-Main-Sequence (PMS) evolution of young stars are
characterized by a substantial interaction between the central star and the surrounding disk …
characterized by a substantial interaction between the central star and the surrounding disk …