OH emission from IRAS sources (Slysh+ 1997)

Details OH emission from IRAS sources (Slysh+ 1997) OH emission from IRAS sources (Slysh+ 1997)

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..41240085s&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/124/85. Originally published in: 1997A&AS..124...85S

Computer Science

Infrared Sources, Masers, Radio Lines

Scientific paper

Results of a continued search for OH main line emission from IRAS sources are reported. Towards a sample of 182 sources which consists of IRAS sources selected by the colour criterion for ultracompact HII region, and several IRAS cores, H2O masers and bipolar outflows, we detected 19 new OH masers of Class I and 5 OH/IR candidates. The correlation between IR and OH maser flux is confirmed. Also 51 thermal and 4 absorption sources were detected. The low radial velocities and derived OH column densities suggest that the thermal OH emission comes from nearby dark clouds. There is evidence that IRAS sources towards which thermal emission was detected are connected with these dark clouds. (2 data files).

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