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    1. Dispersion Measure
    ... 2 components of ISM Hydrogen - disk + halo . Disk . vary with Galactic radius . ... Near sun, . Need to include spiral arms and HII regions . ... Sun at R = 10 kpc , z =0 . Calibrate using other methods . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/pulsar/Tutorial/tut/node34.html -- 3.9 Кб -- 04.02.2013
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    2. http://www.atnf.csiro.au/research/Astro2010/talks/shukurov.pdf
    ... 2 (1µG)2 , C = 2(h/l)2 50, D ( h/v )2 10, the dynamo numb er near the Sun, Dcrit 8, critical dynamo numb er Dep endence of B on SFR, disc-halo connection, winds, galactic evolution, etc. 2 hot Vz = S , S = SFR BS 1/4 (IF all other relevant parameters are ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/Astro2010/talks/shukurov.pdf -- 927.1 Кб -- 16.06.2010
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    3. ATNF Colloquium
    ... sensitive to HI-rich objects in these groups to below 10^7 M(sun) of HI, . ... The HI mass function and the mass function of the luminous halos for the . ... Milky Way and have average HI masses of <4x10^5 M(sun). The spatial . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=534 -- 28.0 Кб -- 01.03.2014
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    4. Main Sequence Stars
    ... log( L / L Sun )= n log( M / M Sun ) or . L/L Sun = ( M/M Sun ) n (Equation 6.1) . ... log( L / L Sun )= n log( M / M Sun ) or . L/L Sun = ( M/M Sun ) n (Equation 6.1) . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/astrophysics/stellarevolution_mainsequence.html -- 75.1 Кб -- 11.04.2016
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    5. Astrophysics and Cosmic Engine Glossary
    ... The laws are: . The planets orbit the Sun in elliptical orbits, with the Sun as one common focus. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/outreach/education/senior/astrophysics/astrophysics_glossary.html -- 92.1 Кб -- 11.04.2016
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    6. http://www.atnf.csiro.au/people/Ray.Norris/papers/n244.pdf
    ... This creates a halo of heated gas called the coma, which is then blown by solar wind in the direction opposite the sun, creating a large dust tail. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n244.pdf -- 256.8 Кб -- 23.09.2010
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    7. http://www.atnf.csiro.au/research/pulsar/array/uploads/Main/0702586.pdf
    ... As the relevant distance D from the Sun is much larger than those between planets and the Sun, the acceleration by the PBH should be regarded as that for the solar system barycenter (SSB). ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/pulsar/array/uploads/Main/0702586.pdf -- 100.3 Кб -- 20.03.2007
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    8. http://www.atnf.csiro.au/pasa/15_2/russell/paper.pdf
    ... the s-process abundances were reminiscent of those found in extreme halo red giants ... Yet RV Tau variables have much higher metallicities than extreme halo stars. ... of stars similar to our own Sun, and the nucleosynthetic processes that occur ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pasa/15_2/russell/paper.pdf -- 107.2 Кб -- 27.07.1998
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    9. http://www.atnf.csiro.au/people/Amy.Kimball/Publications/ivezic_et_al_2006.pdf
    ... C. Allende Prieto6 , R. ґ Wilhelm7 , Y. Sun Lee5 , T. Sivarani5 , M. Juric4 , R ... modeled by three discrete components: the thin disk, the thick disk, and the halo ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Amy.Kimball/Publications/ivezic_et_al_2006.pdf -- 2545.7 Кб -- 02.10.2013
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    10. http://www.atnf.csiro.au/research/Astro2010/abstracts.html
    ... possess radio halos indicating a vertical transport of young accelerate d cosmic-ray electrons from the disc into the halo ... database of Sun's magnetic flux and address the question on whether or not the quiet Sun magnetism follows the sunspot cycle ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/Astro2010/abstracts.html -- 54.9 Кб -- 02.10.2012
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