Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...397l..27s&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 397, no. 1, p. L27-L30.
Astronomy and Astrophysics
Astronomy
16
Active Galactic Nuclei, Galactic Evolution, Infrared Sources (Astronomy), Molecular Gases, Carbon Monoxide, Emission Spectra, Galactic Structure, Interstellar Matter, Red Shift
Scientific paper
Following the paper by Kawabe et al. (1992) the results of aperture synthesis observations of CO(J = 3-2) emission in IRAS F10214 + 4724, with the Nobeyama Millimeter Array (NMA), are reported. CO(J = 3-2) emission is detected only at the blueshifted half of the CO(J = 3-2) velocity range reported in previous single-dish observations; the redshifted half is not detected in our observations. The detected CO(J = 3-2) emission is located at a VLA and optical position and shows a compact shape. This component contains (3-15) x 10 exp 11/sq h solar masses of molecular gas and has a beam deconvolved size 12/h kpc in diameter. The molecular gas surface density is as high as that in infrared luminous galaxies. The nondetected component must have brightness temperatures lower than the sensitivity and is probably extended or composed of a number of subcomponents. The molecular gas distribution suggests that IRAS F10214 + 4724 is an interacting or merging system.
Ishiguro Masato
Ishizuki Sumio
Kawabe Ryohei
Sakamoto Kazushi
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