HD93521 and the local high latitude interstellar medium

Details HD93521 and the local high latitude interstellar medium HD93521 and the local high latitude interstellar medium

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979phdt.........4c&link_type=abstract

Ph.D. Thesis Princeton Univ., NJ.

Other

20

Interstellar Gas, Interstellar Matter, Ultraviolet Spectroscopy, Cosmic Gases, Gas Analysis, Interplanetary Medium, Mapping, O Stars, Spectroscopic Analysis, Spectrum Analysis, Sun

Scientific paper

Ultraviolet spectroscopic observations of the interstellar gas between the sun and the distant, high latitude O star HD93521 were obtained. The column densities of a number of interstellar gaseous species as a function of radial velocity were determined by profile fitting the data, and earlier visual and radio data for this line of sight. The volume densities, gas phase abundances, and other physical conditions parameters of the gas were derived. A comparison with the areal information about the high galactic latitude sky provided by 21 cm mapping, soft X-ray mapping, and the recurrence of particular velocity components in interstellar absorption toward other stars enabled a model for the local high latitude interstellar medium to be formulated.

Affiliated with

Also associated with

No associations

Rating

HD93521 and the local high latitude interstellar medium 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 HD93521 and the local high latitude interstellar medium, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and HD93521 and the local high latitude interstellar medium will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1702830