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    51. http://www.atnf.csiro.au/people/naomi.mcclure-griffiths/Thesis/chap9.ps.gz
    ... The analysis focused on the interaction of massive stars with the ISM. ... and several generations of massive 256 stars involved in the formation of a large ... and determine whether shells on the trailing edges of spiral arms experience a break ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/naomi.mcclure-griffiths/Thesis/chap9.ps.gz -- 103.1 Кб -- 29.09.2001
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    52. Publications
    ... B.S. "Radio observations of HD93129A: the earliest O star with the highest mass loss ... CASWELL, J.L. "OH 1720-MHz masers in southern star-forming regions". ... J.M. & CAMILO, F. "The cosmic coalescence rates for double neutron star binaries ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/newsletter/jun04/Publications.htm -- 60.0 Кб -- 28.02.2014
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    53. http://www.atnf.csiro.au/pasa/17_3/storey/paper.pdf
    ... constructed, and led, among other things, to the discovery of young stars in the LMC ... near-infrared astronomy could become routine: precision photometry of standard stars ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pasa/17_3/storey/paper.pdf -- 53.9 Кб -- 15.03.2001
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    54. http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/cena/CenA.booklet.pdf
    ... The black hole mass measurements of both tracers, gas and stars, are in excellent agreement and provide one of the cleanest gas versus stars comparisons of a BH mass determination. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/cena/CenA.booklet.pdf -- 454.5 Кб -- 22.06.2009
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    55. http://www.atnf.csiro.au/people/Ray.Norris/papers/n220_preprint.pdf
    ... For example, the appearance of a star or constellation can tell people when it's ... people in Arnhem Land know that when the star Spica sets just after the Sun, the ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n220_preprint.pdf -- 548.5 Кб -- 24.04.2008
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    56. http://www.atnf.csiro.au/pub/people/hsim/for_Sarah_Brooker/Captions_info.doc
    ... A long | | | | | |exposure| | | | | |, | | | | | |showing | | | | | |star | | | | | |trails. | | | |cen-a-radio6cm+opt_Burns&Pri|48 KB |Radio |** NOT FOR USE. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pub/people/hsim/for_Sarah_Brooker/Captions_info.doc -- 46.5 Кб -- 07.04.2004
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    57. http://www.atnf.csiro.au/research/LVmeeting/magsys_pres/ruzicka.pdf
    ... i.e. ... ...every fit contained major HI structures trailing stream (Magellanic Stream) leading tail (Leading Arm) in total ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/LVmeeting/magsys_pres/ruzicka.pdf -- 953.1 Кб -- 04.08.2007
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    58. Luminosity dependent changes of pulse profiles in the X-ray binary GX 1+4
    ... Profiles measured during the GX 1+4 high state in the 1970's are all trailing edge bright. ... Keywords: X-rays:stars - accretion discs - pulsars:individual:GX 1+4 . HTML Section . Download Full Paper . б  . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_2/greenhill/paper/index.html -- 52.1 Кб -- 08.04.2016
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    59. http://www.atnf.csiro.au/research/smc_h1/pasa.ps.gz
    ... are seen to correlate with Hff regions, indicating sites of current star formation ... are devoid of optical emission and may represent regions of future star formation ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/smc_h1/pasa.ps.gz -- 641.3 Кб -- 12.05.1998
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    60. D Annotation File Format
    ... FONT hershey12 # Mark the four Trapezium stars with blue circles, and connect them. ... The leading space is ignored, but a trailing space # after "Trap" would not be. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/karma/user-manual/node17.html -- 25.7 Кб -- 13.02.2011
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