in the
Chamaeleontis Cluster Eric E. Mamajek , Warrick A. Lawson , Eric D. Feigelson, PASA, 16 (3), 257.
Footnotes
Use the ``back'' function on your browser to return to the main text where you left it.- ... regions.1
- Note that we include microwave surveys at both 8 and 4.8 GHz in our discussion since the emission from young stars is usually spectrally flat (Güdel & Benz 1993).
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- ... package2
- Documentation on Miriad (Multichannel Image Reconstruction Image Analysis and Display) is available at http://www.atnf.csiro.au/computing/software/miriad, and was written by Bob Sault and Neil Killeen of ATNF.
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- ... galaxy3
- About 0.1 extragalactic source with S > 0.4 mJy are expected by chance to appear in the 10 x 1 arcmin2 regions we examined at 8.4 GHz (Windhorst et al. 1993) while
10 are expected at 5 GHz (Bridle 1989) .
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© Copyright Astronomical Society of Australia 1997
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