Global Model of the Interstellar Medium in Our Galaxy with New Constraints on the Hot Gas Component

Details Global Model of the Interstellar Medium in Our Galaxy with New Constraints on the Hot Gas Component Global Model of the Interstellar Medium in Our Galaxy with New Constraints on the Hot Gas Component

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...497..759f&link_type=abstract

Astrophysical Journal v.497, p.759

Astronomy and Astrophysics

Astronomy

88

Ism: Cosmic Rays, Ism: Bubbles, Ism: General, Ism: Structure, Stars: Supernovae: General

Scientific paper

We model the Galactic distribution of the interstellar gas, cosmic rays, magnetic fields, gravitational field, supernovae, and superbubbles, based on the most recent observational data and on the requirement that the interstellar medium (ISM) be in hydrostatic equilibrium. Our model ISM will be used in a companion paper to compute the filling factor of the hot interstellar gas component as a function of Galactic radius and height.

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