The 157 micron /C II/ emission from NGC 2024 - Core and halo components

Details The 157 micron /C II/ emission from NGC 2024 - Core and halo components The 157 micron /C II/ emission from NGC 2024 - Core and halo components

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...264..538k&link_type=abstract

Astrophysical Journal, Part 1, vol. 264, Jan. 15, 1983, p. 538-542. Research supported by the Aerospace Corp;

Astronomy and Astrophysics

Astronomy

16

Hydrogen Clouds, Infrared Astronomy, Nebulae, Radiative Recombination, Radio Astronomy, Astronomical Maps, Cloud Physics, Continuous Radiation, Cores, Fine Structure, Halos, Line Spectra, Recombination Reactions

Scientific paper

Portions of the nebula NGC 2024 were mapped in the 157 micron (C II) line. Results show the presence of a compact component centered on the radio-recombination line regions and a more extended nebulosity. It is found that the central component emits 157 micron line and continuum fluxes at a level of 4 x 10 to the -16th W/sq cm and 5 x 10 to the -16th W/sq cm (micron), respectively. The continuum emission drops off more rapidly with distance from the peak, although line emission is approximately 30% of the peak value at a distance 18 min to the SE of the peak. In addition, related observations were carried out on M42.

Affiliated with

Also associated with

No associations

Rating

The 157 micron /C II/ emission from NGC 2024 - Core and halo components 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 The 157 micron /C II/ emission from NGC 2024 - Core and halo components, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 157 micron /C II/ emission from NGC 2024 - Core and halo components will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1195981