Figure 8 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 8.

Primary QPO frequency is shown as a function of the ratio of source luminosity to Eddington luminosity. QPO frequency is observed to be monotonically increasing with the source luminosity.

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