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V346 Aquilae / V346 Aql

Picture
Light curve of the EA eclipsing binary V346 Aquilae, constructed from observations made with the Bradford Robotic Telescope Cluster Camera  (BRT) and two primary minima observed from Somerby with a 2" objective lens and Atik Titan Camera.

The results have not been transformed.

Black  BRT 2013 07 02 to 2013 12 06.     Red 2" Titan 2012 08 09   Blue 2" Titan 2012 09 29.
​All observations unfiltered and untransformed.

The best fit period is 1.1064 days (as calculated by Peranso/ANOVA) which compares well with the catalogue value  of 1.106363 days ref AAVSO VSX (accessed 2015 10 01).

The component sets of data are shown below.
​

Picture
Picture
V346 Aquilae primary minimum. 2" Titan, Somerby Observatory, 2012 August 9.
​

Picture
Picture
V346 Aquilae primary minimum.  2" Titan, Somerby Observatory, 2012 September 29.

Picture
BRT observations by date.
Picture
Phase diagram plotted from BRT observations.

Notes

The catalogue values for the period are 1.1063628 d ref GCVS and 1.106363 d ref AAVSO VSX.

A couple of visual observations using my 10" Newtonian.

[ Page updated 15 March 2017 ]
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