Recent Science Highlights
8 April 1995
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Using data from the public archive of the EUVE all-sky survey, Dr.
Antonella Fruscione has systematically searched for short wavelength
(58-174 Å) EUV emission around approximately 2500 distinct positions
in the sky corresponding to known X-ray emitting extragalactic
sources. She finds that twenty X-ray galaxies are EUV bright and were
detected with significance above 4 sigma during the EUVE survey: eight
(six Seyfert galaxies and two BL Lacertae objects) are reported for
the first time as sources of EUV emission. Sixty-eight additional
galaxies are detected with a lower significance (sigma between 3 and
4), but the list is affected by a high percentage of spurious sources.
The paper has been recently submitted to the Astrophysical Journal.
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Dr. Jurgen Schmitt, Dr. Jeremy Drake, and Dr. Robert Stern have
summarized their finding about resonant scattering in a paper recently
submitted to ApJ Letters entitled "EUV Line Emission From Cool Stars:
Resonantly Scattered or Not - That is the Question!". The authors
argue, based upon statistical analysis of fluctuations in the EUVE
spectrum of Procyon and ROSAT X-ray data, that resonance scattering
(as proposed by Dr. Schrijver and collaborators in a paper published
in Astromony and Astrophysics) appears not to be relevant for the
interpretation of the EUV and X-ray spectra of cool inactive stars.
Instead, a number of as yet unidentified spectral lines not included
in current plasma codes produces a false "continuum" in excess of that
predicted.
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