In this thesis, a multi-wavelength study on the cyclic events of η Carinae was performed. The presence of a hole in the polar region of the Homunculus was confirmed by the velocity …
Neste trabalho apresentamos uma análise das observaçoes das linhas de recombinaçao em ondas milimétricas (H30α, H35α, H40α e H50β) na direçao de η Carinae obtidas, entre …
The 6307A emission line in the spectrum of Eta Car (Martin et al. 2006) is blue-shifted [S III] 6313A emission originating from the outer wind structures of the massive binary system. We …
Nesta dissertação são apresentados os resultados obtidos da espectroscopia de campo integral da nebulosa do Homúnculo. As observações foram feitas na banda J, no intervalo …
The Historical Evidence for the 5.52-Year Cycle Page 1 – Eta Carinae at the Millennium ASP Conference Series, Vol. 179, 1999 JA Morse, RM Humphreys, and A. Damineli, eds. The …
The periodic minima in η Carinae are now well defined and interpreted as due to periastron passage of two massive stars in a very eccentric orbit. Different mechanisms have been …
A Damineli, DJ Hillier, MF Corcoran… - Monthly Notices of …, 2008 - academic.oup.com
A full description of the 5.5-yr low excitation events in η Carinae is presented. We show that they are not as simple and brief as previously thought, but a combination of two components …
E Bohm-Vitense, SG Love - … Journal, Part 1 (ISSN 0004-637X) …, 1994 - adsabs.harvard.edu
Abstract For the Cepheid l Carinae, with a pulsation period of 35.5 days, we have studied the emission-line fluxes as a function of pulsational phase in order to find out whether we …
AA de Astronomıa, EM Arnal, A Brunini, JJC Olmedo… - astronomiaargentina.org.ar
Even after more than a century of intensive studies, little is known about η Carinae as a star. Its high luminosity and the observed episodes of mass ejection suggest that it is a LBV …