A spectroscopic study of IRAS F10214 + 4724

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A spectroscopic study of IRAS F10214+4724

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IRAS F10214+4724: the inner 100pc

We use new high resolution near-infrared spectroscopy and our previouslypublished optical spectroscopy of the gravitationally-lensed Seyfert-2 galaxy F10214+4724 to study both the links between the starburst and AGN in this object and the properties of the line-emitting clouds in the inner narrow-line region. Close inspection of the rest-frame UV spectrum reveals interstellar or stellar absorpt...

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The Open University ’ s repository of research publications and other research outputs A spectroscopic study of IRAS F 10214 + 4724

The z 1⁄4 2:286 IRAS galaxy F10214 þ 4724 remains one of the most luminous galaxies in the Universe, despite its gravitational lens magnification. We present optical and near-infrared spectra of F10214 þ 4724, with clear evidence for three distinct components: lines of width ,1000 km s from a Seyfert 2 nucleus; & 200 km s lines which are likely to be associated with star formation; and a broad ...

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Spectroscopic Evidence That the Extreme Properties of Iras F 10214+4724 Are Due to Gravitational Lensing

The extreme bolometric luminosity of IRAS F 10214+4724, and in particular the huge mass in molecular gas inferred from the CO line uxes have led to suggestions that this is a giant galaxy in the process of formation. An arc-like structure and the closeness of a second object suggest, however, that gravitational lensing may be responsible for its anomalously high luminosity and mass. In this pap...

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ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 1998

ISSN: 0035-8711,1365-2966

DOI: 10.1046/j.1365-8711.1998.01522.x