The Central Component of Gravitational Lens Q0957+561
Haarsma, Deborah B.
Winn, Joshua N.
Lehar, JosephNote: Order does not necessarily reflect citation order of authors.
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CitationHaarsma, Deborah B., Joshua N. Winn, Irwin Shapiro, and Joseph Lehár. 2008. The Central Component of Gravitational Lens Q0957+561. The Astronomical Journal 135(3): 984-990.
AbstractIn 1981, a faint radio source (G′) was detected near the center of the lensing galaxy of the famous “twin quasar” Q0957+561. It is still unknown whether this central radio source is a third quasar image or an active nucleus of the lensing galaxy, or a combination of both. In an attempt to resolve this ambiguity, we observed Q0957+561
at radio wavelengths of 13 cm, 18 cm, and 21 cm, using the Very Long Baseline Array
in combination with the phased Very Large Array and the Green Bank Telescope. We
measured the spectrum of G′ for the first time and found it to be significantly different from the spectra of the two bright quasar images. This finding suggests that the central component is primarily or entirely emission from the foreground lens galaxy, but the spectrum is also consistent with the hypothesis of a central quasar image suffering free-free absorption. In addition, we confirm the previously-reported VLBI position of G′ just north of the optical center of the lens galaxy. The position slightly favors the hypothesis that G′ originates in the lens, but is not conclusive. We discuss the prospects
for further clarification of this issue.
Citable link to this pagehttp://nrs.harvard.edu/urn-3:HUL.InstRepos:2634168
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