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 - 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 …
wind binary η Carinae dropped by a factor of 2–3 between 1999 and 2010. We present …
Modelling the asymmetric wind of the luminous blue variable binary MWC 314
A Lobel, JH Groh, C Martayan, Y Frémat… - Astronomy & …, 2013 - aanda.org
Aims. We present a spectroscopic analysis of MWC 314, a luminous blue variable (LBV)
candidate with an extended bipolar nebula. The detailed spectroscopic variability is …
candidate with an extended bipolar nebula. The detailed spectroscopic variability is …
Accretion of dense clumps in the periastron passage of η Carinae
We perform 3D hydrodynamical numerical simulations of the winds interaction process in
the massive binary system η Carinae, and find the secondary star to accrete mass from the …
the massive binary system η Carinae, and find the secondary star to accrete mass from the …
A comprehensive study of supernovae modeling
C Li - 2013 - search.proquest.com
The evolution of massive stars, as well as their endpoints as supernovae (SNe), is important
both in astrophysics and cosmology. While tremendous progress towards an understanding …
both in astrophysics and cosmology. While tremendous progress towards an understanding …