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20142019
most citedThe fossil wind structures of Eta Carinae: changes across on 5.54-year cycle

31 citations · 179 across the 8 of their papers we have counts for

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8 papers · 1 filter

astro-ph.SR2019★ 28 cited

NOEMA maps the CO environment of the red supergiant Cep

M. Montargès, W. Homan, D. Keller +8

Red supergiant stars are surrounded by a gaseous and dusty circumstellar environment created by their mass loss which spreads heavy elements into the interstellar medium. The struc…

astro-ph.SR2018★ 16 cited

Developing a self-consistent AGB wind model: I. Chemical, thermal, and dynamical coupling

Jels Boulangier, Nicola Clementel, Allard Jan van Marle +2

The material lost through stellar winds of Asymptotic Giant Branch (AGB) stars is one of the main contributors to the chemical enrichment of galaxies. The general hypothesis of the…

astro-ph.SR2016★ 31 cited

The fossil wind structures of Eta Carinae: changes across on 5.54-year cycle

Theodore R. Gull, Thomas I. Madura, Mairan Teodoro +11

Eta Carinae, the closest, active, massive binary containing a highly unstable LBV, exhibits expanding, compressed wind shells, seen in emission, that are spatially and spectrally r…

astro-ph.SR2016★ 23 cited

To and beyond! The He I absorption variability across the 2014.6 periastron passage of Carinae

Noel D. Richardson, Thomas I. Madura, Lucas St-Jean +11

We have monitored the massive binary star Carinae with the CTIO/SMARTS 1.5~m telescope and CHIRON spectrograph from the previous apastron passage of the system through the rece…

astro-ph.SR2015★ 16 cited

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

Nicola Clementel, Thomas I. Madura, Chael J. H. Kruip +1

Spectral observations of the massive colliding wind binary Eta Carinae show phase-dependent variations, in intensity and velocity, of numerous helium emission and absorption lines…

astro-ph.SR2015★ 20 cited

3D Printing Meets Computational Astrophysics: Deciphering the Structure of Eta Carinae's Inner Colliding Winds

Thomas I. Madura, Nicola Clementel, Theodore R. Gull +2

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_Sun), highly eccentri…

astro-ph.SR2014★ 28 cited

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

Nicola Clementel, Thomas I. Madura, Chael Kruip +2

The highly eccentric binary system Eta Carinae shows numerous time-variable emission and absorption features. These observational signatures are the result of interactions between…

astro-ph.SR2014★ 17 cited

3D Radiative Transfer in Carinae: Application of the SimpleX Algorithm to 3D SPH Simulations of Binary Colliding Winds

N. Clementel, T. I. Madura, C. J. H. Kruip +2

Eta Carinae is an ideal astrophysical laboratory for studying massive binary interactions and evolution, and stellar wind-wind collisions. Recent three-dimensional (3D) simulations…