000002207 001__ 2207
000002207 005__ 20160701171701.0
000002207 0247_ $$2DOI$$a10.1111/j.1365-2966.2012.21597.x
000002207 037__ $$aASTROimport-364
000002207 100__ $$aJohnstone, R. M.
000002207 245__ $$aHydrogen two-photon continuum emission from the Horseshoe filament in NGC 1275
000002207 260__ $$c2012
000002207 520__ $$aFar-ultraviolet emission has been detected from a knot of Ha emission in the Horseshoe filament, far out in the NGC 1275 nebula. The flux detected relative to the brightness of the Ha line in the same spatial region is very close to that expected from hydrogen two-photon continuum emission in the particle heating model of Ferland et al. if reddening internal to the filaments is taken into account. We find no need to invoke other sources of far-ultraviolet emission such as hot stars or emission lines from C IV in intermediate-temperature gas to explain these data. 
000002207 700__ $$a Canning, R. E. A.
000002207 700__ $$a Fabian, A. C.
000002207 700__ $$a Ferland, G. J.
000002207 700__ $$a Lykins, M.
000002207 700__ $$a Porter, R. L.
000002207 700__ $$a van Hoof, P. A. M.
000002207 700__ $$a Williams, R. J. R.
000002207 773__ $$c1421-1429$$i2$$pMonthly Notices of the Royal Astronomical Society$$v425$$y2012
000002207 85642 $$ahttp://esoads.eso.org/abs/2012MNRAS.425.1421J
000002207 905__ $$apublished in
000002207 980__ $$aREFERD