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    21. http://www.atnf.csiro.au/pub/people/vlbi/vsop/www/vsop_970519.sked.extract
    ... 25 06:00-15:00 L 1055+018 PENT-TI AT HO HH KA VT142 147-TU May 27 07:00-12:30 L 1055+018 MITK-KA UD 1.6/5 GHz pointing on Cygnus A on May 28, May 29 VT800 151-SA May 31/01 19:00-06:30 L 1156+295 SOCR-VLBA EB JB MC NT ON TR WB VT144 153-MO Jun 02 08:00-14 ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pub/people/vlbi/vsop/www/vsop_970519.sked.extract -- 4.8 Кб -- 20.05.1997
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    22. http://www.atnf.csiro.au/research/workshops/2012/ALMA/Hill_ALMAWorkshop2012.pdf
    ... Molecular cloud complexes ! Vela! Mon R1-R2 Rosette! Cygnus X! M16/M17/Sh40! NGC 6334! NGC 6357! W3/KR140! ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/workshops/2012/ALMA/Hill_ALMAWorkshop2012.pdf -- 1775.1 Кб -- 20.03.2012
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    23. Contributions to the project by the Consortium and DRAO
    ... The DRAO ST project is surveying the region , which runs along the Perseus arm in one direction and the Cygnus arm in the other, with an angular resolution of at 1420 MHz. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/english/paper/node1.html -- 56.9 Кб -- 08.04.2016
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    24. http://www.atnf.csiro.au/people/rnorris/papers/n212_final.pdf
    ... Source 3C 273 3C 273 Cygnus-A Cygnus-A Redshift 1 7 1 7 20 cm flux (mJy) 713 4.5 695 1.9 3.6 m flux (Jy) 635 2.8 22 0.04 include k-corrections and are based on a standard cosmology with H0 = 71 km s-1 Mpc-1 , m = 0.27, vac = 0.73. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/rnorris/papers/n212_final.pdf -- 560.0 Кб -- 17.07.2007
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    25. Pulsars and the ISM II
    ... Two surveys of extra-galactic point sources located behind supernova remnants have been ambiguous with no clear evidence for a higher power law index although one group do claim an enhancement behind the Cygnus Loop (Dennison et al.б 1984). ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/17_1/dwarkadas/paper/node5.html -- 54.4 Кб -- 08.04.2016
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    26. Introduction
    ... A region of lesser intensity extends for a few tens of degrees northwards into the AGASA field of view and there is a less convincing enhancement in the Cygnus region of the galactic plane, close to the direction of the inward spiral arm. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/17_3/clay2/paper/node1.html -- 53.1 Кб -- 08.04.2016
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    27. Prospects for multi-wavelength studies of the ISM
    ... In other remnants (e.g. the Cygnus loop, Lozinskaya 1992, especially pp 134-143) there is close correlation in some of the fine structure but also uncorrelated structures, suggesting a diversity of excitation mechanisms in different parts of the remnant. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/cram/paper/node4.html -- 56.9 Кб -- 08.04.2016
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    28. http://www.atnf.csiro.au/people/Enno.Middelberg/pubs/middelberg2005b/middelberg2005b.ps.gz
    ... The sample comprises NGC 1052 (LINER), NGC 4261 (FR I), Centaurus A (FR I), Hydra A (FR I) and Cygnus A (FR II). ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Enno.Middelberg/pubs/middelberg2005b/middelberg2005b.ps.gz -- 113.6 Кб -- 02.06.2004
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    29. ATNF Science Symposium 2007
    ... of about 600 parsecs, similar to the spatial resolution of the famous Virgo A (M87) and Cygnus A images made with the VLA ... of resolution elements, because the radio source is physically so much larger than both Virgo A (80kpc) and Cygnus A (140 kpc ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/conferences/2007/atnf-symposium/abstracts.html -- 63.6 Кб -- 11.04.2016
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    30. http://www.atnf.csiro.au/people/Enno.Middelberg/pubs/middelberg2005b/middelberg2005b.pdf
    ... The sample comprises NGC 1052 (LINER), NGC 4261 (FR I), Centaurus A (FR I), Hydra A (FR I) and Cygnus A (FR I I). ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Enno.Middelberg/pubs/middelberg2005b/middelberg2005b.pdf -- 92.6 Кб -- 02.06.2004
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