[HTML][HTML] Eta Carinae's 2014.6 spectroscopic event: Clues to the long-term recovery from its Great Eruption

A Mehner, K Davidson, RM Humphreys… - Astronomy & …, 2015 - aanda.org
Aims. Every 5.5 years, η Car's light curve and spectrum change remarkably across all
observed wavelength bands. These so-called spectroscopic events are most likely caused …

3D radiative transfer simulations of Eta Carinae's inner colliding winds–I. Ionization structure of helium at apastron

N Clementel, TI Madura, CJH Kruip… - Monthly Notices of …, 2015 - academic.oup.com
The highly eccentric binary system Eta Carinae (η Car) shows numerous time-variable
emission and absorption features. These observational signatures are the result of …

3D radiative transfer simulations of Eta Carinae's inner colliding winds–II. Ionization structure of helium at periastron

N Clementel, TI Madura, CJH Kruip… - Monthly Notices of …, 2015 - academic.oup.com
Spectral observations of the massive colliding wind binary Eta Carinae show phase-
dependent variations, in intensity and velocity, of numerous helium emission and absorption …

3D printing meets computational astrophysics: deciphering the structure of η Carinae's inner colliding winds

TI Madura, N Clementel, TR Gull… - Monthly Notices of …, 2015 - academic.oup.com
We present the first 3D prints of output from a supercomputer simulation of a complex
astrophysical system, the colliding stellar winds in the massive (≳ 120 M⊙), highly eccentric …

The Optical Wind Line Variability of η Carinae During the 2009.0 Event

ND Richardson, DR Gies, TR Gull… - The Astronomical …, 2015 - iopscience.iop.org
We report on high-resolution spectroscopy of the 2009.0 spectroscopic event of η Carinae
collected via SMARTS observations using the CTIO 1.5 m telescope and echelle …

[PDF][PDF] Tratamento de Dados de Radioobservaçoes: Dois Casos

RS Mengato - sites.usp.br
Este trabalho consiste de duas partes. A primeira envolve o estudo dos componentes
ejetados do quasar 3C 273, que foram acompanhados usando técnicas de VLBI em 2 cm …

Orbital Parameters for the Eta Carinae Binary System

A Kashi, N Soker - arXiv preprint arXiv:1508.03576, 2015 - arxiv.org
We show that recent observations of He I and N II lines of $\eta $ Carinae may provide
support for an orbital orientation where the secondary star is closest to us at periastron …