Soft X-ray Emission Line Structure in the Spectra of Accretion-powered Sources: the Importance of Thermal Instability in the Irradiated Gas

Details Soft X-ray Emission Line Structure in the Spectra of Accretion-powered Sources: the Importance of Thermal Instability in the Irradiated Gas Soft X-ray Emission Line Structure in the Spectra of Accretion-powered Sources: the Importance of Thermal Instability in the Irradiated Gas

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994nhxr.conf..627k&link_type=toc

New Horizon of X-Ray Astronomy. First Results from ASCA. Proceedings of the International Conference on X-ray Astronomy, held Ma

Astronomy and Astrophysics

Astronomy

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