Slit and integral-field optical spectroscopy of the enigmatic quasar HE0450-2958
arXiv:0709.3743 · doi:10.1051/0004-6361:20078725
Abstract
Interest in the quasar HE0450-2958 arose following the publication of the non-detection of its expected massive host, leading to various interpretations. This article investigates the gaseous and stellar contents of the system through additional VLT/FORS slit spectra and integral field spectroscopy from VLT/VIMOS. We apply our MCS deconvolution algorithm on slit spectra for the separation of the QSO and diffuse components, and develop a new method to remove the point sources in Integral Field Spectra, allowing extraction of velocity maps, narrow-line images, spatially resolved spectra or ionization diagrams of the surroundings of HE0450-2958. The whole system is embedded in gas, mostly ionized by the QSO radiation field and shocks associated with radio jets. The observed gas and star dynamics are unrelated, revealing a strongly perturbed system. Despite longer spectroscopic observations, the host galaxy remains undetected.
9 pages, 13 figures, in press in A&A
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Cited by in corpus (8)
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- A new twist to an old story: HE 0450-2958, and the ULIRG(optically bright QSO) transition hypothesis
- Study of a homogeneous QSO sample: relations between the QSO and its host galaxy
- GEMINI 3D spectroscopy of BAL+IR+Fe II QSOs: II. IRAS 04505-2958 an explosive QSO with hypershell and a new scenario for galaxy formation and galaxy end
- The QSO HE0450-2958: Scantily dressed or heavily robed? A normal quasar as part of an unusual ULIRG
- Near-IR observations of the HE0450-2958 system: discovery of a second AGN?
- Deep near-infrared imaging of the HE0450-2958 system