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A&A 478, 739-746 (2008)
DOI: 10.1051/0004-6361:20078176
The unusual UV continuum of quasar Ton 34 and the possibility of crystalline dust absorption
L. Binette1, 2 and Y. Krongold11 Instituto de Astronomía, UNAM, Ap. 70-264, 04510 México, DF, México
2 Département de Physique, de Génie Physique et d'Optique, Université Laval, Québec, QC, G1K 7P4, Canada
(Received 27 June 2007/ Accepted 22 November 2007)
Abstract
Context.Luminous quasars are known to display a sharp steepening
of the continuum near 1100 Å. This spectral feature is not well
fitted by current accretion disk models, unless Comptonization of
the disk emission is invoked. Absorption by carbon crystalline dust
has been proposed to account for this feature.
Aims.Ton 34 (
= 1.928)
exhibits the steepest far-UV decline
among the 183 quasar HST-FOS spectra analyzed by Telfer et al.
(2002, ApJ, 565, 773). It is an ideal object to test the crystalline dust
hypothesis as well as alternative interpretations of the UV
break.
Methods.We reconstruct the UV spectral energy distribution of Ton 34 by combining HST, IUE and Palomar spectra.
Results.The far-UV continuum
shows a very deep continuum trough, which is bounded by a steep
far-UV rise. We fit the trough assuming nanodiamond dust
grains.
Conclusions.Extinction by carbon crystalline dust reproduces the deep
absorption trough of Ton 34 reasonably well, but not the observed
steep rise in the extreme UV. We also study the possibility of an
intrinsic continuum rollover. The dust might be part of a high
velocity outflow (
13 000 km s-1), which is observed in
absorption in the lines of C IV
1549, O VI
1035, N V
1240 and Ly
.
Key words: ISM: dust, extinction -- galaxies: quasars: general -- quasars: individual: Ton 34 -- ultraviolet: general
© ESO 2008
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