Clustering of Cold Hydrogen Gas on Protons

Details Clustering of Cold Hydrogen Gas on Protons Clustering of Cold Hydrogen Gas on Protons

Aug 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.223..815c&link_type=abstract

Nature, Volume 223, Issue 5208, pp. 815-816 (1969).

Physics

34

Scientific paper

KRASOVSKII1 has suggested that the presence of ion-clusters of hydrogen in gaseous nebulae could account for the absorption and polarization of stellar radiation. It has since been argued2 that interstellar gas densities are too low for such processes. Hoyle and co-workers3,4 have, however, proposed that condensation of hydrogen on graphite grains at ~3 K might promote the formation of galaxies and stars. The densities of hydrogen in interstellar clouds may thus be great enough for ion-clusters to form by interaction with radiation.

Affiliated with

Also associated with

No associations

Rating

Clustering of Cold Hydrogen Gas on Protons does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Clustering of Cold Hydrogen Gas on Protons, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Clustering of Cold Hydrogen Gas on Protons will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1690350