Observations of young low-mass stars in dense cores

Details Observations of young low-mass stars in dense cores Observations of young low-mass stars in dense cores

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sao..reptq....m&link_type=abstract

Semiannual Status Report, 1 Oct. 1985 - 31 Mar. 1986 Smithsonian Astrophysical Observatory, Cambridge, MA.

Astronomy and Astrophysics

Astronomy

Dust, Gases, Infrared Astronomy, Mapping, C-141 Aircraft, Emission Spectra, Infrared Astronomy Satellite

Scientific paper

In this period the first maps were made during two flights of the Kuipper Airborne Observatory (KAO) in January 1986. One of these shows extended emission at 100 and 160 microns from the dense core B35 containing the IRAS point source 05417+0907. The 160 micron emission has approximately the same extent as the NH3 (1,1) line emission at 1.4 cm, indicating close correspondence between the warm dust and the dense gas. The 160 micron map shows a previously unknown secondary maximum about 90 arcsec north of the IRAS source.

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