Multi-colour optical photometry of V404 Cygni in outburst
J Martí, PL Luque-Escamilla… - Astronomy & …, 2016 - aanda.org
J Martí, PL Luque-Escamilla, MT García-Hernández
Astronomy & Astrophysics, 2016•aanda.orgContext. This observational paper has been prepared in the context of the large multi-
wavelength effort by many observers with the aim of following up the transient flaring event
of V404 Cygni that took place for several weeks in 2015 June. Aims. Our main original aim
was to contribute to the study of this transient source by acquiring broad-band photometric
observations during its most active flaring phases. Nevertheless, after a detailed analysis of
the data, several interesting results were obtained that encouraged a dedicated publication …
wavelength effort by many observers with the aim of following up the transient flaring event
of V404 Cygni that took place for several weeks in 2015 June. Aims. Our main original aim
was to contribute to the study of this transient source by acquiring broad-band photometric
observations during its most active flaring phases. Nevertheless, after a detailed analysis of
the data, several interesting results were obtained that encouraged a dedicated publication …
Context
This observational paper has been prepared in the context of the large multi-wavelength effort by many observers with the aim of following up the transient flaring event of V404 Cygni that took place for several weeks in 2015 June.
Aims
Our main original aim was to contribute to the study of this transient source by acquiring broad-band photometric observations during its most active flaring phases. Nevertheless, after a detailed analysis of the data, several interesting results were obtained that encouraged a dedicated publication.
Methods
The methodology used was based on broad-band differential CCD photometry. This outburst of V404 Cygni rendered the source a very bright target easily within reach of small educational telescopes. Therefore, the 41 cm telescope available at the Astronomical Observatory of the University of Jaén was used in this work.
Results
We detected variability at different time scales, both in amplitude and colour. Individual optical flares appear every half hour on average during our 3 h long observation, although large-amplitude (~1 mag) variations are also observed to occur on intervals as short as 10 min. Also, colour variations appear to be highly correlated in a colour-colour diagram. Another remarkable finding is the detection of time lag, from about one to a fraction of a minute between light curves in different filters (VRcIc).
Conclusions
The observed behaviour is tentatively interpreted in an scenario based on the ejection of non-thermal emitting, relativistic plasmons, with their synchrotron spectra extending up to optical wavelengths. This would render some of the V404 Cygni flares very similar to those of the well-know microquasar GRS 1915+105
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