EXOSAT Observations of the Low-Luminosity X-Ray Burster 4U 0614+091: Evidence for a Hard Power-Law Tail

Details EXOSAT Observations of the Low-Luminosity X-Ray Burster 4U 0614+091: Evidence for a Hard Power-Law Tail EXOSAT Observations of the Low-Luminosity X-Ray Burster 4U 0614+091: Evidence for a Hard Power-Law Tail

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...440..841b&link_type=abstract

Astrophysical Journal v.440, p.841

Astronomy and Astrophysics

Astronomy

19

Stars: Individual Alphanumeric: 4U 0614+09, X-Rays: Bursts, X-Rays: Stars

Scientific paper

We have analyzed archival EXOSAT observations of 4U 0614+091 as recorded by the Medium Energy experiment (2-10 keV). The data set consists of five spectra, all associated with low X-ray luminosities (L(X,1-20 keV) ≤ 2 × 1036 ergs s-1, d = 2 kpc). The spectrum corresponding to the highest intensity state (FX = 3.9 × 10-9 ergs cm-2 s-1) is well fitted by the combination of a steep power law with a photon index of 2.7 and a relatively strong 1.5 keV blackbody component carrying off 25% of the total 1-20 keV luminosity. The two spectra associated with the lowest X-ray fluxes (FX = 1.2, 1.1 × 10-9 ergs cm-2 s-1) are adequately described by the sum of a harder power law (photon index ˜ 1.9) and a cooler blackbody component (˜0.5 keV) carrying of 6% and 10% of the 1-20 keV flux, respectively. Finally, for the two other spectra with slightly larger X-ray fluxes (FX = 1.5 × 10-9 ergs cm-2 s-1), both are best fitted by a single power law (photon index ˜2.1-2.2), and an upper limit of ˜10% on the contribution of any blackbody component with temperature between 0.5 and 1.5 keV has been derived.
4U 0614+091 enlarges the list of X-ray bursters displaying a hard power-law spectrum in X-rays at low- luminosity states, as well as a clear anticorrelation between spectral hardness and intensity. The EXOSAT results show that when the contribution of the blackbody component reaches 25% of the total 1-20 keV flux, the spectrum steepens. This result strengthens the idea that the presence of a strong blackbody emission (most likely originating from the surface of the compact object) may be responsible for the quenching of the high- energy emission in high-luminosity neutron star systems. On the other hand, the same data show also that when the blackbody component contributes, less than ˜10%, it does not affect the high-energy emission of the system.
The EXOSAT results may also account for the fact that 4U 0614+091 was previously detected by HEAO 1 A-4 up to 80 keV, when the source was probably in a very low state. Both the HEAO 1 A-4 and EXOSAT results add support to the hypothesis that X-ray bursters emit low-flux, hard X-ray tails when they reach low-intensity states.

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