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    1. giant_radio_galaxies
    ... Recurrent activity in giant radio galaxies. ... Giant radio galaxies constitute a class of radio sources with linear sizes on the megaparsec scale (Saripalli 1988). ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/newsletter/feb01/untitl10.htm -- 6.8 Кб -- 23.01.2013
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    2. http://www.atnf.csiro.au/research/cena/documents/presentations/struve.pdf
    ... Conference: The many faces of Centaurus A Is Centaurus A a typical Radio Galaxy? ... Australia Why are we interested in Centaurus A? Because it is a Radio Galaxy ... Outline A complete sample of nearby Radio Galaxies (RGs) - large-scale properties ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/cena/documents/presentations/struve.pdf -- 2291.1 Кб -- 16.07.2009
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    3. Radio Sources in the 2dF Galaxy Redshift Survey. I. Radio source populations1
    ... and 60% are active galaxies (mostly low-power radio galaxies and a few Seyferts ... a homogeneous set of around 4000 radio-galaxy spectra, which will be a powerful tool ... radio continuum: galaxies, galaxies: distances and redshifts, galaxies: active ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/16_3/sadler/paper/paper.html -- 51.3 Кб -- 08.04.2016
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    4. ATNF Daily Astronomy Picture
    ... Radio Galaxy Zoo: host galaxies and radio morphologies derived from visual inspection . by Julie Banfield (ANU) . ... We present results from the first twelve months of operation of Radio Galaxy Zoo 75% consensus among the Radio Galaxy Zoo cross ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/ATNF-DailyImage/archive/2015/01-Aug-2015.html -- 5.8 Кб -- 10.04.2016
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    5. Radio Sources in the 2dF Galaxy Redshift Survey. I. Radio source populations1
    ... and 60% are active galaxies (mostly low-power radio galaxies and a few Seyferts ... a homogeneous set of around 4000 radio-galaxy spectra, which will be a powerful tool ... radio continuum: galaxies, galaxies: distances and redshifts, galaxies: active ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/16_3/sadler/paper/index.html -- 52.2 Кб -- 08.04.2016
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    6. http://www.atnf.csiro.au/research/Astro2008/Postings/Mark_Lacy.pdf
    ... High redshift radio galaxies and SMBH evolution Mark Lacy Outline - what did we ... Radio galaxies contain really big black holes. ... Some high-z radio galaxies are forming a lot of stars. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/Astro2008/Postings/Mark_Lacy.pdf -- 2454.2 Кб -- 26.06.2008
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    7. Evolutionary Paths in Galaxy Morphology
    ... The environmental impact on the powerful radio galaxy NGC 612 (PKS 0131-36). ... types of morphological properties of radio galaxies and it remains unclear as to ... this 'nature vs nurture' debate for nearby radio galaxies will provide clues to the ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/conferences/2013/gzo/abstracts/a1.html -- 49.1 Кб -- 11.04.2016
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    8. The giant radio galaxy J0116-473
    ... Australia Telescope National Facility . The giant radio galaxy J0116-473. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/images/astronomical/j0116-473.html -- 47.5 Кб -- 08.04.2016
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    9. Origin of Radio Galaxies Investigated with HI observations and Optical
    ... CSIROpedia . Origin of Radio Galaxies Investigated with HI observations and Optical Spectroscopy - Bjorn Emonts - Lunch Talk . ... In order to investigate this we are studying a complete sample of nearby radio galaxies with HI and optical spectra. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=801 -- 26.9 Кб -- 01.03.2014
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    10. Redshifted H I and OH absorption in radio galaxies and quasars
    ... Publications . Redshifted H I and OH absorption in radio galaxies and quasars . ... cm and OH 18-cm absorption in the hosts of a sample of radio galaxies and quasars, we detect H I in three of the 10 and OH in ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Matthew.Whiting/papers/html_abstracts/absn3_abs.html -- 4.4 Кб -- 05.02.2013
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