X-ray spectral models of Galactic bulge sources - The emission-line factor

Details X-ray spectral models of Galactic bulge sources - The emission-line factor X-ray spectral models of Galactic bulge sources - The emission-line factor

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...326..186v&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 326, March 1, 1988, p. 186-193.

Astronomy and Astrophysics

Astrophysics

16

Emission Spectra, Galactic Bulge, Milky Way Galaxy, X Ray Binaries, X Ray Spectra, Astronomical Models, Goodness Of Fit, Heao 2, Line Spectra

Scientific paper

Current difficulties in finding unique and physically meaningful models for the X-ray spectra of Galactic bulge sources are exacerbated by the presence of strong, variable emission and absorption features that are not resolved by the instruments observing them. Nine Einstein solid state spectrometer (SSS) observations of five Galactic bulge sources are presented for which relatively high resolution objective grating spectrometer (OGS) data have been published. It is found that in every case the goodness of fit of simple models to SSS data is greatly improved by adding line features identified in the OGS that cannot be resolved by the SSS but nevertheless strongly influence the spectra observed by SSS.

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