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1. http://www.mso.anu.edu.au/seminars/abstracts/20160407-1100.html
During the last decade a third window for ground-based astronomy was opened and high energy astrophysics now enables studies up to photon energies of 100 TeV. A wide range of objects were discovered to emit significant amounts of energy in the high-energy gamma-ray regime, including star-forming regions, pulsars, supernova remnants, massive binaries, the diffuse interstellar medium, the Galactic Centre, AGN, etc. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20160407-1100.html -- 4.7 Кб -- 10.04.2016
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2. http://www.mso.anu.edu.au/PSI/
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Ссылки http://www.mso.anu.edu.au/PSI/ -- 1.3 Кб -- 01.10.2012
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3. http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Bizyaev04
... Printed in U.S.A. THE STELLAR DISK THICKNESS OF LOW SURFACE BRIGHTNESS GALAXIES D. Bizyaev 1,2,3 and S. Kajsin 4 Received 2003 October 23; accepted 2004 June 9 ABSTRACT We present surface photometry results for a sample of 11 edge-on galaxies observed with the 6 m telescope at the Special Astrophysical Observatory, Russia. ... We find from a comparison of photometric scales that the stellar disks of LSB galaxies are thinner than those of high surface brightness ( HSB) galaxies. ... UGC 11301 .. ...
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Ссылки http://www.mso.anu.edu.au/~kcf/surya/spiralstructure/Bizyaev04 -- 2057.9 Кб -- 09.07.2007
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