New results about diffuse galactic emission at 380 microns

Details New results about diffuse galactic emission at 380 microns New results about diffuse galactic emission at 380 microns

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.260..161c&link_type=abstract

In ESA Proceedings of an ESA Workshop on a Spaceborne Submillimeter Astronomy Mission. A Cornerstone of the ESA Long Term Scienc

Astronomy and Astrophysics

Astronomy

Balloon-Borne Instruments, Galactic Radio Waves, Submillimeter Waves, Cosmic Dust, Interstellar Matter, Radio Astronomy, Temperature Distribution

Scientific paper

Observations in the submillimeter range of the galactic disk from l=-150 to l=82deg were made with a balloon-borne instrument. In-flight calibration of the instrument was made using Jupiter. The longitude profile obtained exhibits diffuse emission all along the disk with bright peaks associated with resolved sources. The averaged galactic spectrum agrees with a temperature distribution of the interstellar cold dust.

Affiliated with

Also associated with

No associations

Rating

New results about diffuse galactic emission at 380 microns 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 New results about diffuse galactic emission at 380 microns, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New results about diffuse galactic emission at 380 microns will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-892521