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Ultraviolet Isotropic Emission from the Blazar 3C 279

E. Pian·A. Koratkar·L. Maraschi·C. M. Urry·G. Madejski·I. M. McHardy·J. E. Pesce·A. Treves·P. Grandi·C. M. Leach
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Abstract

Archival IUE SWP and HST FOS spectra show the presence of a relatively strong, broad Lyman alpha emission line superposed onto the UV spectral continuum of the blazar 3C 279. As opposed to a factor ~50 variation of the continuum flux during eight years, the emission line did not exhibit significant intensity changes. Simultaneous IUE SWP and LWP spectra of 3C 279 in low emission state are fitted by power-laws of index alpha_nu ~1 (f_nu ~ nu^{-alpha_nu}), significantly flatter than measured during higher states. Our observations suggest that the Lyman alpha line is not powered by the beamed, anisotropic synchrotron radiation which produces the observed continuum in 3C 279, but rather by an unbeamed component characterized by slower and lower amplitude variability. The latter may account for the UV continuum observed during the very low state of January 1993.

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E. Pian, A. Koratkar, L. Maraschi, C. M. Urry, G. Madejski, I. M. McHardy, J. E. Pesce, A. Treves, P. Grandi, C. M. Leach. 1998-05-01. Ultraviolet Isotropic Emission from the Blazar 3C 279. https://arxiv.org/abs/astro-ph/9805005

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