Figure 10 from ASTROSAT/LAXPC REVEALS THE HIGH-ENERGY VARIABILITY OF GRS 1915+105 IN THE χ CLASS

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 10.

Time-lag spectra at ∼2.55 Hz QPO frequencies from two LAXPC units, where lag-spectra of second LAXPC unit (LAXPC20; black points) is computed by choosing the reference band from the first LAXPC unit (LAXPC10) and vice versa (red points). The similarity between these curves and for the combined data (top middle panel of Figure 9) shows that instrumental effects such as dead time are not affecting the results.

Other Images in This Article

Copyright and Terms & Conditions