The periodicity of the η Carinae events

被引:108
作者
Damineli, A. [1 ]
Hillier, D. J. [2 ]
Corcoran, M. F. [3 ,4 ,5 ]
Stahl, O. [6 ]
Levenhagen, R. S. [1 ]
Leister, N. V. [1 ]
Groh, J. H. [1 ]
Teodoro, M. [1 ]
Colombo, J. F. Albacete [7 ]
Gonzalez, F. [8 ]
Arias, J. [9 ]
Levato, H. [8 ]
Grosso, M. [8 ]
Morrell, N. [10 ]
Gamen, R. [8 ]
Wallerstein, G. [11 ]
Niemela, V.
机构
[1] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfericas, BR-05508900 Sao Paulo, Brazil
[2] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA
[3] NASA, Goddard Space Flight Ctr, CRESST, Greenbelt, MD 20771 USA
[4] NASA, Goddard Space Flight Ctr, Xray Astrophys Lab, Greenbelt, MD 20771 USA
[5] Univ Space Res Assoc, Columbia, MD 21044 USA
[6] Univ Heidelberg, ZAH, D-69117 Heidelberg, Germany
[7] UNLP, FCAGLP, Buenos Aires, DF, Argentina
[8] Complejo Astron El Leoncito, San Juan, Argentina
[9] Univ La Serena, Dept Fis, La Serena, Chile
[10] Carnegie Observ, Las Campanas Observ, La Serena, Chile
[11] Univ Washington, Dept Astron, Seattle, WA 98195 USA
关键词
stars : general; stars : individual : eta Carinae; stars : binary;
D O I
10.1111/j.1365-2966.2007.12815.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:1649 / 1656
页数:8
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