On the structure and energetics of quasar broad absorption-line outflows
Autor: | I. Paris, Fred Hamann, H. Herbst, Daniel M. Capellupo |
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Přispěvatelé: | Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS) |
Rok vydání: | 2018 |
Předmět: |
Absorption spectroscopy
Astrophysics::High Energy Astrophysical Phenomena FOS: Physical sciences Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics 01 natural sciences Spectral line quasars: general Ionization 0103 physical sciences Galaxy formation and evolution 010303 astronomy & astrophysics Astrophysics::Galaxy Astrophysics Line (formation) Physics [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] 010308 nuclear & particles physics Astronomy and Astrophysics Quasar Astrophysics - Astrophysics of Galaxies Redshift quasars: absorption lines [SDU]Sciences of the Universe [physics] Space and Planetary Science Astrophysics of Galaxies (astro-ph.GA) Outflow |
Zdroj: | Monthly Notices of the Royal Astronomical Society Monthly Notices of the Royal Astronomical Society, 2019, 483, pp.1808-1828. ⟨10.1093/mnras/sty2900⟩ |
ISSN: | 0035-8711 1365-2966 |
DOI: | 10.48550/arxiv.1810.03686 |
Popis: | Quasar accretion-disk outflows might play an important role in galaxy evolution, but they are notoriously difficult to study due to line saturation and blending problems in the Ly-alpha forest. We circumvent these problems by constructing median composite spectra of diverse broad absorption lines (BALs) and `mini-BALs' in SDSS-III BOSS quasars at redshifts 2.3 < z < 3.5. Sorting by CIV 1549,1551 absorption-line strength with AlIII 1855,1863 as an additional indicator of low ionisations (LoBALs) we find the following: (1) Deeper and broader BALs are accompanied by weaker HeII 1640 emission lines, consistent with softer ionising spectra producing more effective radiative acceleration. (2) PV 1118,1128 absorption is present with resolved ~1:1 depth ratios in all composites from mini-BALs to strong BALs indicating that line saturation, large total column densities log N_H(cm^-2) > 22.7, and large ionisation parameters log U > -0.5 are common. (3) Different observed depths in saturated lines identify inhomogeneous partial covering on spatial scales 3 x 10^5 cm^-3 and maximum radial distances R < 23pc from the quasars. (5) For reasonable actual distances, the median BAL outflow has minimum kinetic energy L_K/L > 0.005(R/1.2pc) sufficient (by some estimates) for feedback to galaxy evolution. (6) LoBAL quasars have the largest median outflow column densities, highest velocities, and weakest HeII 1640 emission in our study; they appear to be at one extreme in a distribution of quasar properties where softer ionising spectra drive more powerful outflows. 23 pages, 8 figures, poor formatting (I don't know why), in press with MNRAS, new version updates some references |
Databáze: | OpenAIRE |
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