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The periodicity of the eta Carinae events

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arxiv 0711.4250 v1 pith:MWJIWOC6 submitted 2007-11-27 astro-ph

classification astro-ph
keywords periodcyclecarinaecombineddataepocheventlast
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abstract

Extensive spectral observations of eta Carinae over the last cycle, and particularly around the 2003.5 low excitation event, have been obtained. The variability of both narrow and broad lines, when combined with data taken from two earlier cycles, reveal a common and well defined period. We have combined the cycle lengths derived from the many lines in the optical spectrum with those from broad-band X-rays, optical and near-infrared observations, and obtained a period length of 2022.7+-1.3 d. Spectroscopic data collected during the last 60 years yield an average period of 2020+-4 d, consistent with the present day period. The period cannot have changed by more than $\Delta$P/P=0.0007 since 1948. This confirms the previous claims of a true, stable periodicity, and gives strong support to the binary scenario. We have used the disappearance of the narrow component of HeI 6678 to define the epoch of the Cycle 11 minimum, T_0=JD 2,452,819.8. The next event is predicted to occur on 2009 January 11 (+-2 days). The dates for the start of the minimum in other spectral features and broad-bands is very close to this date, and have well determined time delays from the HeI epoch.

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  1. Gamma-rays and positrons from Colliding Wind Binaries

    astro-ph.HE 2019-09 conditional novelty 4.0 of 10

    Eta Carinae's gamma-ray emission is tied to hadronic acceleration in its colliding stellar winds, and CTA observations of its orbital variability could map the wind geometry and the injected proton and positron flux.

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