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2013ApJ...773L..16T - Astrophys. J., 773, L16 (2013/August-2)
Detection of the compressed primary stellar wind in η Carinae.
TEODORO M., MADURA T.I., GULL T.R., CORCORAN M.F. and HAMAGUCHI K.
Abstract (from CDS):
A series of three Hubble Space Telescope/Space Telescope Imaging Spectrograph spectroscopic mappings, spaced approximately one year apart, reveal three partial arcs in [Fe II] and [Ni II] emissions moving outward from η Carinae. We identify these arcs with the shell-like structures, seen in the three-dimensional hydrodynamical simulations, formed by compression of the primary wind by the secondary wind during periastron passages.
Abstract Copyright: ∼
Journal keyword(s): binaries: general - stars: individual: η Carinae - stars: massive
Simbad objects: 2
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