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http://www.mso.anu.edu.au/~akarakas/stellar_yields/.
http://www.mso.anu.edu.au/~akarakas/stellar_yields/.
1. Index of /~akarakas/model_data
... reference to the following paper: Karakas Lattanzio (2007, PASA, submitted) Each file contains: 1) pulse number 2) the core mass , Mcore ( Msun ) 3) maximum mass of the intershell convection zone, M_csh ( Msun ) 4) duration of intershell convection , t_csh (years) 5) mass dredged into the envelope, D_dredge ( Msun ) 6) lambda 7) lambda_dup defined by Goriely Mowlavi (= lambda x (DMh/Mpulse) where Mpulse is the maximum ...
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Ссылки http://www.mso.anu.edu.au/~akarakas/model_data/ -- 3.4 Кб -- 01.10.2012
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2. 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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