The mm-to-submm continuum spectra of W 3(OH) and K 3-50A

Details The mm-to-submm continuum spectra of W 3(OH) and K 3-50A The mm-to-submm continuum spectra of W 3(OH) and K 3-50A

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...339..183r&link_type=abstract

Astronomy and Astrophysics, v.339, p.183-186 (1998)

Astronomy and Astrophysics

Astrophysics

3

(Ism:) H Ii Regions, Ism: Individual Objects: K 3-50A, Ism: Individual Objects: W 3(Oh), Radio Continuum: Ism

Scientific paper

{We present a model for the integrated flux density of W 3(OH) and K 3-50A allowing these sources to be used as reliable secondary calibrators between 80 and 800 GHz. Using new narrow-band continuum measurements between 86-245 GHz with the 30m telescope and reasonable assumptions about the source sizes, we construct continuum spectra from the mm-to-submm range which are in very good agreement with previously published data. With the fit parameters given in this paper, observers at any single-dish telescope will be able to calculate the expected flux densities of the two sources at any given aperture and frequency.}

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