UV Spectroscopy of Chimneys in Edge-On Galaxies

Details UV Spectroscopy of Chimneys in Edge-On Galaxies UV Spectroscopy of Chimneys in Edge-On Galaxies

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7562d&link_type=abstract

HST Proposal ID #7562

Computer Science

Hst Proposal Id #7562 Interstellar Matter

Scientific paper

Theory predicts the cycling of interstellar material through the galactic Halo. Hot gas and dust from SN in the galaxy disk is confined by the ISM from expanding in the plane, and is pushed preferentially into the halo. The gas may be as hot as 100, 000 K and as it expands will cool. The IS medium near the column or chimney will exhibit the spectrum of the cooler material. This proposal searches for the emissions from the hot component in the UV, looking for OVI, Si IV, CIV lines in emission.

Affiliated with

Also associated with

No associations

Rating

UV Spectroscopy of Chimneys in Edge-On Galaxies 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 UV Spectroscopy of Chimneys in Edge-On Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UV Spectroscopy of Chimneys in Edge-On Galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-895921