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    1. Heiles Symposium Presentations
    ... Warm ionized material & disk/halo interaction (Chair: R. Reynolds) . Hot interstellar material (Chiars: D. Cox & R. Shelton) . ... P. Frisch - Warm partially ionized interstellar gas at the Sun . ...
    [ Сохраненная копия ]  Ссылки http://www.naic.edu/~astro/heiles/Scientific_Presentations.html -- 7.2 Кб -- 23.08.2006
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    2. The Pleiades
    ... ago, making them 1/50th the age of our sun, and they lie some 130 parsecs (425 light ... are still 40 times brighter than our own sun would appear at a similar distance, and ...
    [ Сохраненная копия ]  Ссылки http://www.naic.edu/~gibson/pleiades/ -- 29.7 Кб -- 07.02.2015
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    3. http://www.naic.edu/alfa/ealfa/meeting1/talks/giovanelli.pdf
    ... sun = 9.94 - 2 в log h70 [Mpc**-3 dex**-1] = -1.53 Source-to-beam extent Integration time in sec Signal width in km · The reliability of a detection depends on S/N. Model the probability p, that a "detection" at given S/N will be confirmed, as · Model W ...
    [ Текст ]  Ссылки http://www.naic.edu/alfa/ealfa/meeting1/talks/giovanelli.pdf -- 564.8 Кб -- 08.05.2006
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    4. VIRGOHI 21
    ... Newton Telescope , that it was a dark halo that does not contain the expected bright ... would include any galaxy with a luminosity of less than 10 8 times that of the Sun ... Universe Today . Phys.Org . The Sun (paywall) . ...
    [ Сохраненная копия ]  Ссылки http://www.naic.edu/~rminchin/virgohi21.shtml -- 11.8 Кб -- 09.04.2016
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    5. http://www.naic.edu/alfa/galfa/docs/aoprpsep03_galfa_test.ps.gz
    ... We wish to perform this experiment once during the night and, also, several times during the daytime with the Sun at di erent elevations so that we can get a feel for the Sun's e ect. ...
    [ Текст ]  Ссылки http://www.naic.edu/alfa/galfa/docs/aoprpsep03_galfa_test.ps.gz -- 139.7 Кб -- 05.02.2004
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    6. I-GALFA Reveals Dynamic Events in Our Galaxy
    ... sin(b) | to emphasize disk-halo structure. ... detailed view of gas dynamics within the Galactic disk and coupling into the halo ... spiral arm, the next arm inside the Sun's orbit around the Galactic center ...
    [ Сохраненная копия ]  Ссылки http://www.naic.edu/~gibson/galfa/igalfa/gallery/dyn/ -- 7.1 Кб -- 15.12.2009
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    7. I-GALFA View of a Galactic Tangent Region
    ... away (1 kpc = 3,300 light years), lying between our Sun's orbit around the Galactic center and the Sagittarius spiral arm, the ...
    [ Сохраненная копия ]  Ссылки http://www.naic.edu/~gibson/galfa/igalfa/gallery/tan/ -- 4.6 Кб -- 25.01.2010
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    8. http://www.naic.edu/vscience/schedule/tpfiles/KannappantagA2671tp.ps
    ... that ``cold'' ionized gas accretion may be the predominant fuel for galaxy growth in dark matter halos below a critical mass ... and clustering for all #1500 galaxies down to baryonic mass # 10 9 M sun within 53,000 cubic Mpc of the nearby cosmic web ...
    [ Текст ]  Ссылки http://www.naic.edu/vscience/schedule/tpfiles/KannappantagA2671tp.ps -- 98.3 Кб -- 13.10.2011
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    9. http://www.naic.edu/~astro/highlights/GALFA/galfa_fvw.pdf
    ... Its distance from the Sun would be less than 5.0 kpc or greater than 8.3 kpc. ... It seems to be similar to the halo cloud of Lockman (2002) in the sense that it exists near tangent velocity and shows a clump ...
    [ Текст ]  Ссылки http://www.naic.edu/~astro/highlights/GALFA/galfa_fvw.pdf -- 166.4 Кб -- 20.12.2005
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    10. http://www.naic.edu/~tghosh/a1724/402
    ... halos: Theoretical models suggest a significant amount of matter should be=20 detectable in small dwarf halos nearby to larger ...
    [ Сохраненная копия ]  Ссылки http://www.naic.edu/~tghosh/a1724/402 -- 61.8 Кб -- 25.04.2004
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