Constraints on decreases in η Carinae's mass-loss from 3D hydrodynamic simulations of its binary colliding winds

Monthly Notices of the Royal Astronomical Society, 2013 - academic.oup.com
Recent work suggests that the mass-loss rate of the primary star ηA in the massive colliding
wind binary η Carinae dropped by a factor of 2–3 between 1999 and 2010. We present …

[PDF][PDF] Constraints on decreases in η Carinae's mass loss from 3D hydrodynamic simulations of its binary colliding winds

TI Madura, TR Gull, AT Okazaki… - arXiv preprint arXiv …, 2013 - info-quest.org
Recent work suggests that the mass-loss rate of the primary star ηA in the massive colliding
wind binary η Carinae dropped by a factor of 2− 3 between 1999 and 2010. We present …

Constraints on decreases in Eta Carinae's mass loss from 3D hydrodynamic simulations of its binary colliding winds

TI Madura, TR Gull, AT Okazaki, CMP Russell… - arXiv preprint arXiv …, 2013 - arxiv.org
Recent work suggests that the mass-loss rate of the primary star (Eta A) in the massive
colliding wind binary Eta Carinae dropped by a factor of 2-3 between 1999 and 2010. We …

Constraints on decreases in η Carinae's mass-loss from 3D hydrodynamic simulations of its binary colliding winds

TI Madura, TR Gull, AT Okazaki… - Monthly Notices of …, 2013 - ieeexplore.ieee.org
Recent work suggests that the mass-loss rate of the primary star η A in the massive colliding
wind binary η Carinae dropped by a factor of 2–3 between 1999 and 2010. We present …

[PDF][PDF] Constraints on decreases in η Carinae's mass loss from 3D hydrodynamic simulations of its binary colliding winds

TI Madura, TR Gull, AT Okazaki, CMP Russell… - arXiv preprint arXiv …, 2013 - Citeseer
Recent work suggests that the mass-loss rate of the primary star ηA in the massive colliding
wind binary η Carinae dropped by a factor of 2− 3 between 1999 and 2010. We present …

[PDF][PDF] Constraints on decreases in η Carinae's mass loss from 3D hydrodynamic simulations of its binary colliding winds

TI Madura, TR Gull, AT Okazaki… - arXiv preprint arXiv …, 2013 - academia.edu
Recent work suggests that the mass-loss rate of the primary star ηA in the massive colliding
wind binary η Carinae dropped by a factor of 2− 3 between 1999 and 2010. We present …

[PDF][PDF] Constraints on decreases in η Carinae's mass loss from 3D hydrodynamic simulations of its binary colliding winds

TI Madura, TR Gull, AT Okazaki… - arXiv preprint arXiv …, 2013 - researchgate.net
Recent work suggests that the mass-loss rate of the primary star ηA in the massive colliding
wind binary η Carinae dropped by a factor of 2− 3 between 1999 and 2010. We present …

Constraints on decreases in η Carinae's mass-loss from 3D hydrodynamic simulations of its binary colliding winds

TI Madura, TR Gull, AT Okazaki… - Monthly Notices of …, 2013 - ui.adsabs.harvard.edu
Recent work suggests that the mass-loss rate of the primary star η A in the massive colliding
wind binary η Carinae dropped by a factor of 2-3 between 1999 and 2010. We present …

[PDF][PDF] Constraints on decreases in η Carinae's mass-loss from 3D hydrodynamic simulations of its binary colliding winds

TI Madura, TR Gull, AT Okazaki, CMP Russell… - MNRAS, 2013 - core.ac.uk
Recent work suggests that the mass-loss rate of the primary star ηA in the massive colliding
wind binary η Carinae dropped by a factor of 2–3 between 1999 and 2010. We present …

[引用][C] Constraints on decreases in η Carinae's mass-loss from 3D hydrodynamic simulations of its binary colliding winds

TI Madura, TR Gull, AT Okazaki, CMP Russell… - Monthly Notices of the …, 2013 - cir.nii.ac.jp
Constraints on decreases in η Carinae's mass-loss from 3D hydrodynamic simulations of its
binary colliding winds | CiNii Research CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] …