Study Of The Flux Emitted From The Outer Surface Of The Stars Aldebaran Fomalhaut And Rigel Observed From Nagarkot Observatory Nagarkot Nepal

We present a study on the relative flux density emitted from the outer surface of the stars Aldebaran and Fomalhaut as observed from the Nagarkot Observatory Nepal on the 24th of November 2016. We found that the variation of the relative flux density of the stars were found to be symmetrical in nature going from the outer surface of the star to the interior of the star and finally to the outer surface of the star again through the diameters. The flux was found to be minimum at the outer surface reaching to its maximum in the interior of the star and finally to its minimum value at the outermost surface of the star. The values of the relative flux density were found to be minimum for Rigel and maximum for Aldebaran. There was a slight anomaly detected in the relative flux density of Fomalhaut which may have been due to the debris of dust that surrounds the star.