Fig. 1 from Ultraviolet and Multiwavelength Variability of the Blazar 3C 279: Evidence for Thermal Emission

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

Ultraviolet and Multiwavelength Variability of the Blazar 3C 279: Evidence for Thermal Emission

Authors: E. Pian, C. M. Urry, L. Maraschi, G. Madejski, I. M. McHardy, A. Koratkar, A. Treves, L. Chiappetti, P. Grandi, R. C. Hartman, H. Kubo, C. M. Leach, J. E. Pesce, C. Imhoff, R. Thompson, and A. E. Wehrle

Pian et al. 1999 The Astrophysical Journal 521 112.

Provider: AAS Journals

Caption: Fig. 1.

Multiwavelength light curves of 3C 279 in 1992 December–1993 January, showing (a) dereddened optical R‐band fluxes (from Grandi et al. 1996); (b) dereddened IUE fluxes at 2600 Å; and (c) deabsorbed fluxes at 1 keV for Galactic ﹩N_{\mathrm{H}\,\,{}^{{\rm{\small I}}}}=2.22\times 10^{20}﹩ cm⁻² (from Sambruna 1997). Error bars represent 1 σ uncertainties.

Other Images in This Article

Copyright and Terms & Conditions