W.J. Lang , M.R.W. Masheder, PASA, 15 (1), 70
The html and gzipped postscript versions of this paper are in preprint form.
To access the final published version, download the pdf file.
Next Section: Observations
CO Observations of the -Orionis Ring
W.J. Lang
M.R.W. Masheder
H.H. Wills Physics Laboratory, Bristol University, Tyndall Ave, Bristol, U.K, BS8 1TL
w.j.lang@bristol.ac.uk, mike.masheder@bristol.ac.uk
Abstract:
We present results from a new CO(J=) survey of the -Orionis region. The observations cover 110 square degrees uniformly on a Nyquist-sampled grid. We discover CO-emission at levels far lower than possible in previous surveys, revealing a structure similar to that seen in IRAS 100 maps. We derive a total molecular mass of б 1.110 M. A possible explanation for the isolated and localised outbreak of star-formation in the region is discussed.
Keywords: ISM: bubbles -- ISM:clouds -- ISM:HII regions -- ISM: molecules
HTML Section | Download Full Paper |
---|---|
б© Copyright Astronomical Society of Australia 1997
ASKAP
Public