Analysis of IUE observations of the galactic corona and the existence of molecular clouds in the halo

Details Analysis of IUE observations of the galactic corona and the existence of molecular clouds in the halo Analysis of IUE observations of the galactic corona and the existence of molecular clouds in the halo

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.196..527h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 196, Aug. 1981, p. 527-532.

Astronomy and Astrophysics

Astronomy

12

Coronas, Cosmic Gases, Gas Ionization, Iue, Magnetohydrodynamic Waves, Molecular Clouds, Absorption Spectra, Abundance, Gas Cooling, Magellanic Clouds, Satellite Observation

Scientific paper

IUE observations of ions in the galactic corona are reanalyzed and Savage and de Boer's (1979) conclusion that the detected hot phase has a temperature proportional to 80,000 K is confirmed. The cold phase must be at a temperature of less than 24,000 K and probably contains substantial amounts of molecular material. Molecules, such as CH(+), OH and SH, may exist in detectable abundances in the transition regions between the hotter gas and the cold gas on the far sides of halo molecular clouds.

Affiliated with

Also associated with

No associations

Rating

Analysis of IUE observations of the galactic corona and the existence of molecular clouds in the halo 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 Analysis of IUE observations of the galactic corona and the existence of molecular clouds in the halo, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analysis of IUE observations of the galactic corona and the existence of molecular clouds in the halo will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1747613