… Unless otherwise noted, the following discussion in Sections 5.1-5.4 is from the work of
Raymond and Shull & McKee. Most of the relevant collisional and radiative rates can be found …

… interfaces between the clouds and hot gas (McKee and Cowie 1 977), which depends on …
do not have space to dominate the dynamics of the SNR (see Cowie, McKee, and Ostriker …

The interstellar medium is intermittently disturbed by violent events supernova explosions
being but one example-which cause large increases in the local pressure. As the result of the …

… McKee (1979) to estimate the physical conditions at that point, and we then follow the …
For v~ = 100 km s' we use the results of Shull and McKee (1979): the photon flux between …

X rays emitted in the inner part of an accretion disk system can heat the surface of the disk
farther out, producing a corona and possibly driving off a strong wind. The dynamics of …

Heats of formation, molecular geometries, ionization potentials, and dipole moments, calculated
by the MNDO method, are reported for a wide variety of boron compounds. The results …

A model compound approach to oxidized hemocyanin is described. The essential structural
features of diamagnetism, 3.6-A copper-copper separation, approximate tetragonal …

3 6 Á. hemocyanin the collective evidence from vibrational, 1· 1 2 magnetic, 3 chemical, 4
and electronic1· 4· 5 data requires a dinuclear copper (II) site having endogeneous and …

The inter- and intracellular regulator nitric oxide (NO) has been suggested to play a role in
the modulation of cellular excitability, but the mechanism(s) by which this occurs remain …

… Even if bond fission is assisted by a concerted rearrangement to the more stable isomer
CH2=SH+, the energy required should still be greater than that corresponding to formation of the …