... CSIRO Fellow Ron Ekers and Helen Sim describes not only the "Oh-my-God" particle, a particle from space - probably the nucleus of an iron atom with the energy of a well-bowled cricket ball, but also neutrinos and using the Moon as a neutrino detector ...
... and supernova remnants Masers, Galactic structure and the Galactic Centre Masers in AGN env ironments Masers and starburst activ ity Diagnostics and interpretation in extragalactic env ironments New mm and sub-mm masers Future facilities Inv ited speakers ...
Ralph Sutherland RSAA, ANU, ANITA Cooling in the ISM Cooling in the ISM Example: Nearby RGs with Resolved Hosts M87 Sparkes et al 2004 astro-ph/0402204 Example: Active Galaxies: Cen A Example: Equilibrium Heating and Cooling : HII regions...
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Ссылки http://www.atnf.csiro.au/whats_on/workshops/comp2005/talks/sutherland.pdf -- 1638.2 Кб -- 13.05.2005 Похожие документы
... around 6.4 keV is likely to be contaminated with unpulsed iron line emission. б б ... 4 summed over energies from 3-10 keV , excluding the data from around the iron line ...
... differences between the RV Tau variable iron abundances and those of the local ... Certainly there is no suggestion of an over abundance of iron. ... There is also no sign of an underabundance in s-process elements relative to iron. ...