Connection between Radio and X-ray emission in Microquasar GRS 1915+105

Details Connection between Radio and X-ray emission in Microquasar GRS 1915+105 Connection between Radio and X-ray emission in Microquasar GRS 1915+105

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...20313902f&link_type=abstract

American Astronomical Society Meeting 203, #139.02; Bulletin of the American Astronomical Society, Vol. 36, p.585

Astronomy and Astrophysics

Astronomy

Scientific paper

Relatively stronger low-frequency (0.1-10 Hz) QPOs in X-ray emission was found associated with higher radio flux. The radio flux is low when power density spectrum (PDS) of X-ray emission is dominated by continuum. This implies that the low-frequency (0.1-10 Hz) QPOs are related to energy transfer from accretion disk to corona or jet, which is consistent with accretion ejection instability (AEI) model, whereas the magnetic rotation instability (MRI) may produce the continuum component in PDS. The correlation between X-ray properties (PDS and energy spectrum) and radio flux will be reported and implication of the connection between disk and ejection is discussed.

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