The periodicity of the eta Carinae events
Contribuinte(s) |
UNIVERSIDADE DE SÃO PAULO |
---|---|
Data(s) |
19/10/2012
19/10/2012
2008
|
Resumo |
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 P(pres) = 2022.7 +/- 1.3 d. Spectroscopic data collected during the last 60 yr yield an average period of P(avg) = 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 He I 6678 to define the epoch of the Cycle 11 minimum, T(0) = JD 245 2819.8. The next event is predicted to occur on 2009 January 11 (+/- 2 d). The dates for the start of the minimum in other spectral features and broad-bands are very close to this date, and have well-determined time-delays from the He I epoch. |
Identificador |
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v.384, n.4, p.1649-1656, 2008 0035-8711 http://producao.usp.br/handle/BDPI/27040 10.1111/j.1365-2966.2007.12815.x |
Idioma(s) |
eng |
Publicador |
WILEY-BLACKWELL |
Relação |
Monthly Notices of the Royal Astronomical Society |
Direitos |
restrictedAccess Copyright WILEY-BLACKWELL |
Palavras-Chave | #stars : general #stars : individual : eta Carinae #stars : binary #2003.5 MINIMUM #HOMUNCULUS NEBULA #SPECTROSCOPY #VARIABILITY #INTERFEROMETRY #EMISSION #SPECTRA #BINARY #EJECTA #Astronomy & Astrophysics |
Tipo |
article original article publishedVersion |