An extended far-infrared emission complex at IC 1318b and IC 1318c

Details An extended far-infrared emission complex at IC 1318b and IC 1318c An extended far-infrared emission complex at IC 1318b and IC 1318c

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...247..530c&link_type=abstract

Astrophysical Journal, Part 1, vol. 247, July 15, 1981, p. 530-539.

Astronomy and Astrophysics

Astronomy

19

Astronomical Maps, Far Infrared Radiation, Infrared Astronomy, Nebulae, Continuous Radiation, Cosmic Dust, Cosmic Gases, Ionized Gases, Nonthermal Radiation, Radio Sources (Astronomy), Supernova Remnants

Scientific paper

A map of extended 90 micron emission with 15 arcmin resolution is presented for sources centered on IC 1318b and c. A strong correlation is found between far-infrared emission and radio continuum emission, although a comparison of far-infrared and CO molecular line maps shows no similarity. Extended far-infrared sources have inferred gas densities, which implies that far-infrared emitting dust is mixed with the ionized gas. Far-infrared emission from dust is also observed in the nonthermal radio source DR 4 which is part of a supernova remnant, and the data are compatible with a core-halo model for the compact source DR 7.

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