Aperture synthesis observations of galactic atomic hydrogen in the direction l=333.5 deg, b=-9,3

Details Aperture synthesis observations of galactic atomic hydrogen in the direction l=333.5 deg, b=-9,3 Aperture synthesis observations of galactic atomic hydrogen in the direction l=333.5 deg, b=-9,3

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.226..173f&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 226, May 1, 1987, p. 173-185.

Astronomy and Astrophysics

Astronomy

2

Galactic Structure, Hydrogen Atoms, Radio Telescopes, Synthetic Apertures, Absorption Spectra, Astronomical Maps, Galactic Radio Waves, H Ii Regions, Milky Way Galaxy, Radio Spectra

Scientific paper

Galactic atomic hydrogen has been mapped with the Parkes two-element synthesis telescope (TEST) in the direction l = 333°.5, b = -0°.3. H I structure on a large angular scale is probed using absorption measurements toward eight compact continuum sources scattered over an area 25 arcmin across. The detailed H I absorption over the extended (4 arcmin) H II region G 333.6-0.2 is mapped with 39×56 arcsec resolution. Various explanations for the 'anomalous' high-velocity gas associated with G 333.3-0.4 are considered in the light of the observations.

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