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    1. The HI bubble surrounding the Wolf-Rayet star WR 149
    ... Neutral hydrogen observations with the Effelsberg 100-m telescope have disclosed an HI bubble surrounding the WN6-7 star WR 149, located in the far side of the Perseus spiral arm. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Baerbel.Koribalski/publications/wrbubbles.html -- 2.3 Кб -- 23.12.2007
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    2. ATNF Media Release - 20 August 1998
    ... That pull is now tearing them apart, by tugging harder on their near side than on their far side. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/multibeam/nature200898.html -- 6.5 Кб -- 02.10.2012
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    3. http://www.atnf.csiro.au/people/naomi.mcclure-griffiths/Thesis/chap4.ps.gz
    ... The far edge of GSH 304-00-12 is at the near side of the arm and opens into the ... The caps of the shell, on both the near and far sides are not readily detected. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/naomi.mcclure-griffiths/Thesis/chap4.ps.gz -- 960.9 Кб -- 29.09.2001
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    4. Galactic Bar
    ... In this model, stars from the near side of the bar lens stars from the far side. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/17_1/yock/paper/node3.html -- 51.3 Кб -- 08.04.2016
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    5. http://www.atnf.csiro.au/nca/WG2.3%20report.pdf
    ... and characterize emerging active regions on the far side of the sun, as well as to ... rely on improved near and far side helioseismological imaging techniques, modelling ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/nca/WG2.3%20report.pdf -- 2925.2 Кб -- 20.09.2005
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    6. http://www.atnf.csiro.au/people/Tasso.Tzioumis/sms2014/Program_draft1-10.pdf
    ... Meens (CNES Space RA observations, Far Side of the Moon, L2 point ................. Langston (NSF Active sensing from space .. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Tasso.Tzioumis/sms2014/Program_draft1-10.pdf -- 420.8 Кб -- 20.02.2014
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    7. http://www.atnf.csiro.au/observers/apply/Legacy_EOI--dense_gas_Breen_et_al.pdf
    ... Specifically, we will: · Characterise the dense gas structure of our Galaxy through sensitive carbon monosulfide (CS) and ammonia (NH3 ) obser vations, allowing us to detect molecular clouds out to the far side of the Galaxy. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/observers/apply/Legacy_EOI--dense_gas_Breen_et_al.pdf -- 77.0 Кб -- 10.03.2016
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    8. http://www.atnf.csiro.au/research/masermeeting/web_papers/505_Richards.pdf
    ... Fractional ionisaton ~10 Linear pol seen from near side only Pol. from far side scrambled? ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/masermeeting/web_papers/505_Richards.pdf -- 1536.0 Кб -- 13.03.2007
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    9. ATNF Colloquium
    ... cores delineate spiral arms, and we have discovered the heretofore missing segment of the Scutum-Centaurus arm on the far side of the Galaxy; (2) compelling evidence for changing physical and chemical conditions of star-forming clumps as they evolve from ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=1242 -- 27.3 Кб -- 01.03.2014
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    10. ATNF Colloquium
    ... The first science run (10 days in January) yielded 60 new sources, including some which must lie on the far side of the Galaxy (from their radial velocities), at distances of at least 16kpc. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=574 -- 27.2 Кб -- 01.03.2014
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