Figure 3 from ASTROSAT/LAXPC REVEALS THE HIGH-ENERGY VARIABILITY OF GRS 1915+105 IN THE χ CLASS

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ASTROSAT/LAXPC REVEALS THE HIGH-ENERGY VARIABILITY OF GRS 1915+105 IN THE χ CLASS

Authors: J S Yadav, Ranjeev Misra, Jai Verdhan Chauhan, P C Agrawal, H M Antia, Mayukh Pahari, Dhiraj Dedhia, Tilak Katoch, P. Madhwani, R K Manchanda, B Paul, Parag Shah, and C H Ishwara-Chandra

2016 The Astrophysical Journal 833 27.

Provider: AAS Journals

Caption: Figure 3.

Square root of disk blackbody normalization (top panel) and the percentage fraction of the disk to the total flux as a function of the Eddington ratio (bottom panel) are shown for different observations. For computing the Eddington ratio, we used a black hole mass of ﹩12.5M\odot ﹩ and a distance to the source D = 9 kpc (Reid et al. 2014).

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