... present, and that the excess mass (above the background density) is 2 10 15 ф M ... in the ACO 3627 cluster, which has a mass of 10 15 M (Woudt 1998; Bohringer et al ...
7. http://www.atnf.csiro.au/pasa/15_1/sabalisck/paper.pdf
... Arsenault, R., Roy, J. R., & 23 Beckman, J. E., Rozas, M., 15, 83 Rozas, M., Beckman, J. E., 307, 735 Terlevich, R., & Melnick, J. Boulesteix, J. 1990, A&A, 234, & Knapen, J. H. 1998, PASA, & Knapen, J. H. 1996, A&A, 1981, MNRAS, 195, 839 Astronomical ...
8. Parkes 50th Anniversary: Programme
... Baerbel Koribalski . PDF . M.P. 14:30-15:00 . The rise of multibeam astronomy . Lister Staveley-Smith . PDF . ... Dave Jauncey . PDF . D.M. 10:15-11:00 . Parkes: the Fulcrum of Southern Hemisphere VLBI . John Reynolds . PDF . ...
9. http://www.atnf.csiro.au/pasa/17_3/hidas/paper.pdf
... transmission spectra are shown in Figures 36, for the wavelength ranges 2 6 µm, 515 µm, 1560 µm and 50500 µm, respectively ... of emission and transmission spectra with varying water vapour content in the mid-IR, from 5 to 15 µm, as for Figure 3 ...
10. H Observations and Data Reduction
... S. Kim , L. Staveley-Smith , R.J. Sault , M.J. Kesteven , D. McConnell , M.A. Dopita , M. Bessell, PASA, 15 (1), 132 . ... Each 15 m pixel corresponds to 20.''63 on the sky, giving a total field size of square. ...