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    • 1 | 2 | След.

    1. Distribution of Young Stars
    ... Given the identification of these filaments with the Orion-Eridanus Bubble (Brown et al. 1995), this is evidence for star formation triggered by some event causing compression of the primordial -Ori GMC along its southern edge. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/lang/paper/node4.html -- 51.8 Кб -- 08.04.2016
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    2. HIPASS galaxy catalogue (HICAT) animations
    ... Hydra (Hya), Centaurus (Cen), Fornax (For), Eridanus (Eri), Pavo (Pav), and Indus ... The Fornax-Eridanus cluster, mostly in green at about 1500 km/s (z = 0.005, 20 Mpc ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Mark.Calabretta/animations/index.html -- 31.0 Кб -- 23.12.2007
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    3. Graduate_students
    ... to Meryl Waugh on the successful submission of her University of Melbourne PhD thesis on "Neutral hydrogen in Fornax and Eridanus - blind basketweaving for beginners", and Ilana Klamer on the successful submission of her University of Sydney PhD thesis on ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/newsletter/oct06/Graduate_students.htm -- 50.1 Кб -- 09.04.2016
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    4. http://www.atnf.csiro.au/pasa/15_1/reynolds/paper.pdf
    ... of the filamentary features are associated with the Orion­ Eridanus bubble (Reynolds & Ogden 1979; Sivan 1974), which fills the ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/reynolds/paper.pdf -- 233.8 Кб -- 14.05.1998
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    5. http://www.atnf.csiro.au/projects/askap/ASKAP_EarlyScience_Workshop_August5th2013.pdf
    ... an ASKAP ADE12 early science case for the HI imaging of Eridanus, a supergroup of galaxies which are in the process of becoming ... Eridanus is a system of 3 in falling groups. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/projects/askap/ASKAP_EarlyScience_Workshop_August5th2013.pdf -- 126.4 Кб -- 01.08.2013
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    6. http://www.atnf.csiro.au/research/multibeam/papers/kilborn_scc_2002.ps.gz
    ... of the Fornax wall is present, and the Eridanus void can be seen to the bottom left ... 3999 km s 1 the Pavo spur is quite obvious, and the Eridanus void is still present ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/multibeam/papers/kilborn_scc_2002.ps.gz -- 448.5 Кб -- 20.06.2002
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    7. http://www.atnf.csiro.au/pasa/15_1/lang/paper.pdf
    ... Given the identification of these filaments with the Orion-Eridanus Bubble (Brown, Hartmann & Button 1995), this is evidence for star formation triggered by some event causing compression of the primordial -Ori GMC along its southern edge. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/lang/paper.pdf -- 341.6 Кб -- 14.05.1998
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    8. Early Results
    ... of the filamentary features are associated with the Orion-Eridanus bubble (Reynolds & Ogden 1979; Sivan 1976), which fills the ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/reynolds/paper/node3.html -- 67.7 Кб -- 08.04.2016
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    9. Atlas of Images
    ... IRAS . From Sutherland & Bally . 15b . Orion-Eridanus . BO3 . Hasselb . suth . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/17_2/bessell/paper/node2.html -- 84.7 Кб -- 08.04.2016
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    10. Photometry Questions
    ... The star нµ Eridanus has an apparent visual magnitude of V = 3.73 and an apparent blue magnitude of B = 4.61. a) What is its colour index? . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/astrophysics/photometry_questions.html -- 66.6 Кб -- 11.04.2016
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