The stellar coronal component of the Galaxy. I - The X-COUNT numerical model

Details The stellar coronal component of the Galaxy. I - The X-COUNT numerical model The stellar coronal component of the Galaxy. I - The X-COUNT numerical model

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...256...86f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 256, no. 1, p. 86-94.

Astronomy and Astrophysics

Astronomy

38

Milky Way Galaxy, Stellar Composition, Stellar Coronas, X Ray Astronomy, Astronomical Models, Color-Magnitude Diagram, Interstellar Extinction

Scientific paper

We present a computational model for the prediction and analysis of the distribution of galactic X-ray stellar coronal source counts, based on models for the distribution of stars and of interstellar hydrogen in the Galaxy and on known properties of stellar X-ray emission in the solar neighborhood. The model can be, and has been used, for comparisons with unbiased X-ray surveys (equivalent to the deep source counts conducted in the optical), for predictions of stellar X-ray observations with new instruments and to estimate the stellar contribution to the X-ray background.

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