GX 339-4 in transition from the hard state

Details GX 339-4 in transition from the hard state GX 339-4 in transition from the hard state

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2545....1m&link_type=abstract

The Astronomer's Telegram, #2545

Astronomy and Astrophysics

Astronomy

8

X-Ray, Request For Observations, Binaries, Black Holes

Scientific paper

The latest RXTE/PCA observation of the black-hole candidate GX 339-4 (2010 April 10, 05:56UT) shows clear evidence that the source is leaving the low-hard state. The power-density spectrum is dominated by two broad-band components with characteristic frequencies around 1 Hz and 9 Hz, on which a narrow QPO with centroid 1.1 Hz is visible. Both components are consistent with the evolution at higher frequencies of features observed previously in the hard state (see Atel 2523).

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