Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...196.2601w&link_type=abstract
American Astronomical Society, 196th AAS Meeting, #26.01; Bulletin of the American Astronomical Society, Vol. 32, p.710
Astronomy and Astrophysics
Astrophysics
Scientific paper
We present aperture synthesis observations of HI (21 cm) line radiation toward the Perseus molecular cloud complex, obtained with the aperture synthesis telescope of the Dominion Radio Astrophysical Observatory (DRAO). Comparison of the HI maps to existing CO maps of the dense cloud complex demonstrates a clear relationship between the molecular and the atomic components. There is a general atomic halo surrounding the molecular cloud, perhaps taking the form of a general outflow. The HI structure is clearly seen to have been affected by recent star formation activity. This work was carried out in part at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA.
Andersson Bengt-Goran
Knee Lewis
Moriarty-Schieven Gerald H.
Wannier Peter G.
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