... IPS Array-Rajkot . 7 0 є 56 ' . 22 є 18 ' . 103 M . ? . S . Mauritius . MRT . ...
2. http://www.atnf.csiro.au/people/naomi.mcclure-griffiths/Thesis/biblio.ps.gz
... 1025 Roberts, W. W. & Hausman, M. A. 1984, ApJ, 277, 744 Rodgers, A. W., Campbell, C. T., & Whiteoak, J. B. 1960, MNRAS, 121, 103 Rozyczka, M. & Tenorio-Tagle, G. 1995, MNRAS, 274, 1157 Saken, J. M., Shull, J. M., Garmany, C. D., Nichols-Bohlin, J., & A ...
3. http://www.atnf.csiro.au/research/electronics/docs/dfc/DFCHandout.pdf
... W ith M of order 103 these represent considerable savings in cost and complexity. ...
4. http://www.atnf.csiro.au/whats_on/workshops/mm_science2001/talks/Rudnitskij.pdf
... State University, Russia Millimetre Science with the Upgraded Australia Telescope 1 Late- type Variables · Red giant stars, M ~ 1 to a few M¤, L ~ a few 103 L¤, · Brightness varies at timescales of tens and hundreds of days, due to stellar pulsations ...
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5. References
... K., Humble, J.E., Fenton, A.G., Fenton K.B. & Duldig, M.L. 1998a JGR 103, 367 ... Lovell, J.L., Duldig, M.L. & Humble, J.E. 1998 JGR 103, 23733 . ... Nagashima, K., Fujimoto, K. & Jacklyn, R.M. 1998 JGR 103, 17429 . ...
6. http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/posters/IAU212-ngc1741.pdf
... W e have chosen four different models: those with metallicity Z/Z=1 and 0.25, and with a total mass of M/M= 103 and 106. ...
7. References
... Franco, J., Tenorio-Tagle, G., Bodenheimer, P., & Rozyczka, M.б 1991, PASP, 103, 803 . ...
8. http://www.atnf.csiro.au/people/rnorris/papers/n159.ps.gz
... 103 Gabuzda D. C., Cawthorne T. V., Roberts D. H., Wardle J. F. C., 1992, ApJ, 388, 40 Gilbert J. A., Conway R. G., 1970, Nat ...