Recurrence of the blue wing enhancements in the high-ionization lines of SDSS 1004+4112A

被引:18
作者
Gomez-Alvarez, P.
Mediavilla, E.
Munoz, J. A.
Arribas, S.
Sanahez, S. F.
Oscoz, A.
Prada, F.
Serra-Ricart, M.
机构
[1] Inst Astrofis Canarias, E-38200 San Cristobal la Laguna, Spain
[2] Univ Valencia, Dept Astron & Astrophys, E-46100 Burjassot, Spain
[3] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[4] European Space Agcy, Estec, Space Telescope Div, NL-2200 AG Noordwijk, Netherlands
[5] CSIC, E-28006 Madrid, Spain
[6] CSIC, Inst Astrofis Andalucia, E-18008 Granada, Spain
[7] Astrophys Inst Potsdam, D-14482 Potsdam, Germany
[8] Ctr Astron Hispano Aleman, Calar Alto Observ, E-04044 Almeria, Spain
关键词
gravitational lensing; quasars : emission lines; quasars : individual (SDSS 1004+4112);
D O I
10.1086/506147
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present integral field spectroscopic observations of the quadruple-lensed QSO SDSS 1004 + 4112 taken with the fiber system INTEGRAL at the William Herschel Telescope on 2004 January 19. In 2003 May, a blueward enhancement in the high-ionization lines of SDSS 1004 + 4112A was detected, and then it faded. Our observations are the first to note a second event of similar characteristics less than 1 year after. Although initially attributed to microlensing, the resemblance among the spectra of both events and the absence of microlensing-induced changes in the continuum of component A are puzzling. The lack of a convincing explanation under the microlensing or intrinsic variability hypotheses makes the observed enhancements particularly relevant, calling for close monitoring of this object.
引用
收藏
页码:L5 / L8
页数:4
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