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    11. http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L09/newplanets.py
    ... Stars interacting gravitationally # Program uses numpy arrays for high speed computations wid=900 heit=600 Nplanets = 100 ... stars try: # numpy r = pos-pos[:,newaxis] # all pairs of star-to-star vectors for n in range(Nplanets+1): r[n,n] = 1e6 ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L09/newplanets.py -- 5.4 Кб -- 30.06.2009
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    12. http://www.mso.anu.edu.au/seminars/abstracts/20150409-1100.html
    ... Albert Zijlstra . "Life in retirement: old stars in old stellar populations". ... Sun-like stars end their lives in a phase of catastrophic mass loss. ... Between 30% and 80% of the mass of the star is lost in an extreme stellar wind. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150409-1100.html -- 4.9 Кб -- 10.04.2016
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    13. COALA - Computational Astrophysics Laboratory
    ... Planetary Science . Planet and Star Formation. ... the angular momentum transport required for star/planet formation remain poorly ... general enough (the presence of a companion star) or not to work at all (convection ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/coala/planet.html -- 3.9 Кб -- 01.10.2012
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    14. http://www.mso.anu.edu.au/~wood/lectures2009/Pulsation_1.pdf
    ... stars · Linear adiabatic pulsation theory => periods of pulsation · Linear non ... stars LITERATURE SOURCES Cox, J P & Giuli, R T 1968, Principles of Stellar Structure ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~wood/lectures2009/Pulsation_1.pdf -- 1998.4 Кб -- 26.03.2009
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    15. http://www.mso.anu.edu.au/seminars/abstracts/20150213-1400.html
    ... An Even More Universal Star Formation Law in Molecular Clouds and Galaxies". ... a system which governs the formation of stars in the dense cores of the interstellar ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150213-1400.html -- 6.3 Кб -- 10.04.2016
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    16. http://www.mso.anu.edu.au/seminars/abstracts/20150205-1100.html
    ... The results provide further evidence that the Galactic halo contains a population of stars accreted from dwarf galaxies and we find that AGB stars were able to contribute to the chemical evolution of the earliest dwarf galaxies. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150205-1100.html -- 6.1 Кб -- 10.04.2016
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    17. http://www.mso.anu.edu.au/seminars/abstracts/20150512-1100.html
    ... How are popular star formation rate indicators affected by the recent star formation history of a galaxy? ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150512-1100.html -- 4.7 Кб -- 10.04.2016
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    18. http://www.mso.anu.edu.au/seminars/abstracts/20160301-1100.html
    ... stars at a given epoch is dependant on many different processes such as: i) in-situ star-formation rates, ii) merger rates, iii ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20160301-1100.html -- 5.5 Кб -- 10.04.2016
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    19. Cepheid Variables
    ... CEPHEID VARIABLE STARS: A Cepheid variable or Cepheid is a member of a particular class of very luminous, massive variable stars with pulsation periods of 1-70 days. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~jerjen/researchprojects/cepheids/cepheids.html -- 8.3 Кб -- 02.10.2012
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    20. http://www.mso.anu.edu.au/seminars/abstracts/20151027-1100.html
    ... I will present the first 2D maps of the star formation rates across AGN host galaxies without contamination from the AGN, and the first maps of the narrow line region emission without contamination from star formation. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151027-1100.html -- 4.8 Кб -- 10.04.2016
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