1. The isolated neutron star RBS1774 revisited ***
- Author
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Schwope, A. D., Erben, T., Kohnert, J., Lamer, G., Steinmetz, M., Strassmeier, K., Zinnecker, H., Bechtold, J., Diolaiti, E., Fontana, A., Gallozzi, S., Giallongo, E., Ragazzoni, R., De Santis, C., Testa, V., Schwope, A. D., Erben, T., Kohnert, J., Lamer, G., Steinmetz, M., Strassmeier, K., Zinnecker, H., Bechtold, J., Diolaiti, E., Fontana, A., Gallozzi, S., Giallongo, E., Ragazzoni, R., De Santis, C., and Testa, V.
- Abstract
We report optical B-band observations with the Large Binocular Telescope (LBT) of the isolated neutron star RBS1774. The stacked image with a total exposure of $2\fh5$reveals a candidate optical counterpart at mB= 26.96 ±0.20 at position $\alpha {\rm (2000)} = {\rm 21^h43^m03\fs40}$, $\delta{\rm (2000)} = +06\degr54^\prime17\farcs5$, within the joint Chandra and XMM-Newton error circles. We analyse archival XMM-Newton observations and derive revised spectral and positional parameters. The predicted optical flux from the extrapolated X-ray spectrum is likely twice as high as reported before. The measured optical flux exceeds the extrapolated X-ray spectral flux by a factor ${\sim}40$(15-60 at 1σconfidence). We interpret our detection and the spectral energy distribution as further evidence of a temperature structure over the neutron star's surface and present a pure thermal model reflecting both the SED and the pulsed fraction of the light curve.
- Published
- 2009
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