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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



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ID: 448198.0, MPI für Astronomie / Publikationen_mpia
Gemini 3D spectroscopy of BAL+IR+FeII QSOs - II. IRAS 04505-2958, an explosive QSO with hypershells and a new scenario for galaxy formation and galaxy end phase
Authors:Lipari, S.; Bergmann, M.; Sanchez, S. F.; Garcia-Lorenzo, B.; Terlevich, R.; Mediavilla, E.; Taniguchi, Y.; Zheng, W.; Punsly, B.; Ahumada, A.; Merlo, D.
Language:English
Date of Publication (YYYY-MM-DD):2009
Journal Abbrev.:Monthly Notices of the Royal Astronomical Society
Volume:398
Issue / Number:4
Start Page:658
End Page:700
Review Status:not specified
Audience:Not Specified
Abstract / Description:From a study of broad absorption line (BAL) + infrared (IR) + FeII quasi-stellar objects (QSOs) [using deep Gemini Multi-Object Spectrograph Integral Field Unit (GMOS-IFU) spectroscopy], new results are presented for IRAS 04505-2958. Specifically, we have studied in detail the outflow (OF) process at two large galactic scales: (i) two blobs/shells at radius r ~ 1.1 and 2.2 kpc, and (ii) an external hypergiant shell at r ~ 11 kpc. In addition, the presence of two very extended hypergiant shells at r ~ 60-80 kpc is also discussed. From this GMOS study the following main results were obtained. (i) For the external hypergiant shell, the kinematics GMOS maps of the ionized gas ([OII], [NeIII], [OIII], Hβ) show a small-scale bipolar OF, with similar properties to those observed in the prototype of exploding external supershells: NGC 5514. (ii) Three main knots - of this hypershell S3 - show the presence of a young starburst. (iii) The two internal shells show OF components with typical properties of nuclear shells. (iv) The two blobs and the hypershell are aligned at PA ~ 131° showing bipolar OF shape at ~10-15 kpc scale. In addition, the more external shells (at ~60-80 kpc scale) are aligned at PA ~ 40° also with bipolar OF shape (perpendicular to the more internal OF). (v) A strong blue continuum and multiple emission-line components were detected in all the GMOS fields. The new GMOS data show a good agreement with an extreme + explosive OF scenario for IRAS 04505-2958, in which part of the interstellar medium (ISM) of the host galaxy was ejected (in multiple shells). This extreme
Free Keywords:ISM: bubbles; galaxies: individual: IRAS 04505-2958; quasars: absorption lines; galaxies: starburst
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2009MNRAS.398..658L [ID No:1]
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