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Far-infrared and radio observations of DR 6, DR 7, and DR 22

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/164325· OSTI ID:7259423
Far-infrared maps are presented for three young H II regions in the Cygnus X region. DR 6 and 7 were mapped in the wavelength band from 40 to 250 microns at 1 arcmin resolution, while DR 22 was mapped in the same band and also at 100-250 microns, providing dust temperature and optical depth information. New VLA maps of these sources are also presented. It is concluded that DR 6 and 7 are powered by clusters of late O or early B type stars, with ages 100,000 yr or less, while DR 22 appears to be produced by a single O6 ZAMS star. Existing (C-12)O maps suggest that the formation of these objects occurred near the edges of molecular clouds. 24 references.
Research Organization:
E. O. Hulburt Center for Space Research, Washington, DC; Sachs/Freeman Associates, Inc., Bowie, MD; Colby College, Waterville, ME; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA; NASA, Goddard Space Flight Center, Greenbelt, MD
OSTI ID:
7259423
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 306; ISSN ASJOA
Country of Publication:
United States
Language:
English