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Astron. Astrophys. 327, 61-71

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Optical-IUE observations of the gamma-ray loud BL Lacertae object S5 0716+714: data and interpretation*

G. Ghisellini1, M. Villata2, C.M. Raiteri2, S. Bosio3, G. De Francesco2, G. Latini3, M. Maesano4, E. Massaro4, F. Montagni4, R. Nesci4, G. Tosti5, M. Fiorucci5, E. Pian6, L. Maraschi7, A. Treves8, A. Comastri9, and M. Mignoli9

1Osservatorio Astronomico di Brera, via Bianchi, 46, I-22055 Merate, Italy
2Osservatorio Astronomico di Torino, I-10025 Pino Torinese, Italy
3Università di Torino, via Giuria 1, Torino, Italy
4Istituto Astronomico, Università di Roma, Unità GIFCO-CNR Roma I, via Lancisi 29, Roma, Italy
5Osservatorio Astronomico, Università di Perugia, Perugia, Italy
6Space Telescope Science Institute, Baltimore, USA
7Osservatorio di Brera, via Brera, 28, Milano, Italy
8International School for Advanced Studies, Trieste, Italy
9Osservatorio Astronomico di Bologna, Italy

Received 31 October 1996 / Accepted 3 June 1997


We monitored the BL Lac object S5 0716+714 in the optical band during the period November 1994 - April 1995, which includes the time of a FORMULA-ray observation by the Energetic Gamma Ray Experiment Telescope (EGRET) on February 14-28, 1995. The light curves in the R and B bands show fast fluctuations superimposed on longer timescale variations. The color index correlates with intensity during the rapid flares (the spectrum is flatter when the flux is higher), but it is rather insensitive to the long term trends. Over the 5 month observational period the light curve shows an overall brightening of about 1 mag followed by a fast decline. The EGRET pointing covers part of the very bright phase (FORMULA) and the initial decline. An ultraviolet spectrum was also obtained with the International Ultraviolet Explorer (IUE) (1200-3000 Å) during the EGRET observations. The variability of the optical emission of S5 0716+714 by itself sets important constraints on the magnetic field strength and on the physical processes responsible for it. Interpreting the whole electromagnetic spectrum with synchrotron self Compton models leads to the prediction of a bright FORMULA-ray state during the EGRET pointing. We discuss how the FORMULA-ray data could be used as a diagnostic of the proposed models. 1

Key words: BL Lac objects: general - BL Lac objects: individual: S5 0716+714 - gamma-rays: theory - ultraviolet: galaxies

*Table 2 is only available in electronic form at CDS via anonymous ftp to cdsarc.u-strasbg.fr ( or via http://cdsweb.u-strasbg.fr/Abstract.html

1Table 2 is only available in electronic form at CDS via anonymous ftp to cdsarc.u-strasbg.fr ( or via http://cdsweb.u-strasbg.fr

Send offprint requests to: G. Ghisellini

© European Southern Observatory (ESO) 1997

Online publication: October 1, 1997
Last change: April 8, 1998