Sylvie F. Beaulieu , Michael A. Dopita, PASA, 15 (1), 144
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: Discussion Title/Abstract Page: A Survey for new Previous Section: Spectroscopy Follow-up | Contents Page: Volume 15, Number 1 |
Comparison with COBE
Using the COBE/DIRBE 1.25, 2.2 and 3.5
m images, we found that there is no significant difference between the longitude distribution of the PNe and the COBE light in the zone of our deep survey. Also, we find that the extinction in our surveyed fields is not severe and that its distribution is fairly uniform. A two-tailed K-S test show that there is no significant difference between the longitude distribution of the PNe and the COBE light in the zone of our deep survey.
| Next Section: Discussion Title/Abstract Page: A Survey for new Previous Section: Spectroscopy Follow-up | Contents Page: Volume 15, Number 1 |
© Copyright Astronomical Society of Australia 1997 ASKAP
Public