Subaru Deep Spectroscopy of a Star-forming Companion Galaxy of BR 1202-0725 at
arXiv:astro-ph/0409273 · doi:10.1086/425887
Abstract
We present deep spatially-resolved optical spectroscopy of the NW companion galaxy of the quasar BR 1202-0725 at . Its rest-frame UV spectrum shows star-forming activity in the nuclear region. The Ly emission profile is symmetric with wavelength while its line width is unusually wide (FWHM km s) for such a high- star-forming galaxy. Spectrum taken along the Ly nebula elongation, which is almost along the minor axis of the companion host galaxy, reveals that off-nuclear Ly nebulae have either flat-topped or multi-peaked profiles along the extension. All these properties can be understood in terms of superwind activity in the companion galaxy. We also find a diffuse continuum component around the companion, which shows similar morphology to that of Ly nebula, and is most likely due to scattering of the quasar light at dusty halo around the companion. We argue that the superwind could expel dusty material out to the halo region, making a dusty halo for scattering.
11 pages, 5 figures, to appear in AJ
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- Varying [CII]/[NII] line ratios in the interacting system BR1202-0725 at z=4.7
- BR1202-0725: An Extreme Multiple Merger at z = 4.7
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- Spitzer Observations of High Redshift QSOs
- Close companions to two high-redshift quasars
- Herschel/PACS far-infrared photometry of two z>4 quasars
- Constraining the Nature of Two Ly-alpha Emitters detected by ALMA at z = 4.7
- The Ionised- and Cool-Gas Content of The BR1202-0725 System as seen by MUSE and ALMA
- Grisms Developed for FOCAS
- ALMA [NII] 205 micron Imaging Spectroscopy of the Interacting Galaxy System BRI 1202-0725 at Redshift 4.7
- K band SINFONI spectra of two SMGs: upper limits to the un-obscured star formation from [O II] optical emission line searches