@Article{TeodoroDHRMSRGMPWCPFGHHNAJLLPBCCHGHW:2016:COOREL,
author = "Teodoro, M. and Damineli, A. and Heathcote, B. and Richardson, N.
D. and Moffat, A. F. J. and St-Jean, L. and Russell, C. and Gull,
T. R. and Madura, T. I. and Pollard, K. R. and Walter, F. and
Coimbra, A. and Prates, R. and Fern{\'a}ndez-Lajus, E. and Gamen,
R. C. and Hickel, G. and Henrique, W. and Navarete, F. and
Andrade, T. and Jablonski, Francisco Jos{\'e} and Luckas, P. and
Locke, M. and Powles, J. and Bohlsen, T. and Chini, R. and
Corcoran, M. F. and Hamaguchi, K. and Groh, J. H. and Hillier, D.
J. and Weigelt, G.",
affiliation = "{NASA Goddard Space Flight Center} and {Universidade de S{\~a}o
Paulo (USP)} and {SASER Team} and {Universit{\'e} de
Montr{\'e}al} and {Universit{\'e} de Montr{\'e}al} and
{Universit{\'e} de Montr{\'e}al} and {NASA Goddard Space Flight
Center} and {NASA Goddard Space Flight Center} and {NASA Goddard
Space Flight Center} and {University of Canterbury} and {Stony
Brook University} and {Laborat{\'o}rio Nacional de Astrofica} and
{Laborat{\'o}rio Nacional de Astrofica} and {Universidad Nacional
de la Plata} and {Universidad Nacional de la Plata} and
{Universidade Federal de Itajub{\'a} (UNIFEI)} and {Universidade
Federal de Itajub{\'a} (UNIFEI)} and {Universidade de S{\~a}o
Paulo (USP)} and {Universidade de S{\~a}o Paulo (USP)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {SASER
Team} and {SASER Team} and {SASER Team} and {SASER Team} and
{Ruhr-Universitat Bochum} and {NASA Goddard Space Flight Center}
and {NASA Goddard Space Flight Center} and {Geneva Observatory}
and {University of Pittsburgh} and {Max-Planck-Institut f{\"u}r
Radioastronomie}",
title = "He II \λ4686 EMISSION from the MASSIVE BINARY SYSTEM in
\η CAR: CONSTRAINTS to the ORBITAL ELEMENTS and the NATURE
of the PERIODIC MINIMA",
journal = "Astrophysical Journal",
year = "2016",
volume = "819",
number = "2",
pages = "131",
month = "Mar.",
keywords = "binaries: general, circumstellar matter, stars: individual
(\ν,,Carinae), stars: massive.",
abstract = "Eta Carinae (\η Car) is an extremely massive binary system
in which rapid spectrum variations occur near periastron. Most
notably, near periastron the He ii \λ4686 line increases
rapidly in strength, drops to a minimum value, then increases
briefly before fading away. To understand this behavior, we
conducted an intense spectroscopic monitoring of the He ii
\λ4686 emission line across the 2014.6 periastron passage
using ground- and space-based telescopes. Comparison with previous
data confirmed the overall repeatability of the line equivalent
width (EW), radial velocities, and the timing of the minimum,
though the strongest peak was systematically larger in 2014 than
in 2009 by 26%. The EW variations, combined with other
measurements, yield an orbital period of 2022.7 ±0.3 days. The
observed variability of the EW was reproduced by a model in which
the line flux primarily arises at the apex of the wind-wind
collision and scales inversely with the square of the stellar
separation, if we account for the excess emission as the companion
star plunges into the hot inner layers of the primary's
atmosphere, and including absorption from the disturbed primary
wind between the source and the observer. This model constrains
the orbital inclination to 135°-153°, and the longitude of
periastron to 234°-252°. It also suggests that periastron passage
occurred on days). Our model also reproduced EW variations from a
polar view of the primary star as determined from the observed He
ii \λ4686 emission scattered off the Homunculus nebula.",
doi = "10.3847/0004-637X/819/2/131",
url = "http://dx.doi.org/10.3847/0004-637X/819/2/131",
issn = "0004-637X and 1538-4357",
language = "en",
targetfile = "Teodoro_he II.pdf",
urlaccessdate = "27 abr. 2024"
}