RX J185635-3754: The EUVE Observation

We observed this target with EUVE for 580 ksec in June and July 1997. The target was easily detected in the DSS. This immer portion of the DSS image subtends 39 arcmin on the sky; this represents only the first 195 ksec of the observation. The three-lobed structure is an instrumental effect.

As expected, the dispersed spectrum is weak, and we are still working on the optimal spectral extraction.

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