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  • 1 | 2 | След.

    1. Limits on the Star Formation Rates of z>2 Damped Ly Systems from H Spectroscopy
    ... are the fully-formed galactic-disk counterparts of today's massive spiral galaxies ... is probably much higher than the space density of spiral galaxies today ... are the counterparts of today's spiral galaxies the associated H emission should be ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node36.html -- 20.9 Кб -- 12.06.2006
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    2. The Co-Addition Technique Applied to Images of Galaxy Cores
    ... Many ellipticals and bulges of spiral galaxies show central, unresolved sources which are particularly bright in the UV and significantly less conspicuous or even completely absent in the corresponding visual images. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/zeilingerw.html -- 10.8 Кб -- 12.06.2006
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    3. http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.pdf
    ... Many ellipticals and bulges of spiral galaxies show central, unresolved sources which are particularly bright in the UV and significantly less conspicuous or even completely absent in the corresponding visual images. ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.pdf -- 49.4 Кб -- 12.06.2006
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    4. HST-NICMOS Observations of Galactic Bulges: Red Nuclei in Nearby Galaxies
    ... Bulges of spiral galaxies are generally seen as small elliptical galaxies in the center of a large spiral. ... and early-type spirals, is a suitable environment for the formation of young stars, and that galaxies, even early-types, are ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node30.html -- 26.7 Кб -- 12.06.2006
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    5. http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.ps.gz
    ... Many ellipticals and bulges of spiral galaxies show central, unresolved sources which are particularly bright in the UV and significantly less conspicuous or even completely absent in the corresponding visual images. ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.ps.gz -- 76.9 Кб -- 12.06.2006
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    6. An Infrared Camera Reduction/Analysis Package
    ... Several barred spiral galaxies and galactic HII regions associated with small molecular clouds were observed with the IR-Camera on the 1.5 m Carlos S?nchez Telescope (CST) on the Teide Observatory during October 1996. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/chans.html -- 7.3 Кб -- 12.06.2006
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    7. http://www.stecf.org/coordination/esa_eso/alma-herschel/report.pdf
    ... 27 6.5 Normal Spirals and Low Surface Brightness Galaxies ..................................... 28 6.6.1 Protostars.. ... Brightness (LSB) and Dwarf Galaxies are among the most common spiral galaxies ...
    [ Текст ]  Ссылки http://www.stecf.org/coordination/esa_eso/alma-herschel/report.pdf -- 1000.5 Кб -- 04.09.2008
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    8. http://www.stecf.org/conferences/adass/adassVII/reprints/chans.pdf
    ... Introduction Several barred spiral galaxies and galactic H ii regions associated with small molecular clouds were observed with the IR-Camera on the 1.5 m Carlos Sanchez ґ Telescope (CST) on the Teide Observatory during October 1996. ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/chans.pdf -- 202.1 Кб -- 12.06.2006
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    9. http://www.stecf.org/conferences/adass/adassVII/reprints/chans.ps.gz
    ... Introduction Several barred spiral galaxies and galactic H ii regions associated with small molecular clouds were observed with the IRнCamera on the 1.5 m Carlos SТanchez Telescope (CST) on the Teide Observatory during October 1996. ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/chans.ps.gz -- 344.8 Кб -- 12.06.2006
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    10. Investigating the Evolution of Quasar Host Galaxies with NICMOS
    ... luminosity AGN display marked preferences in terms of host type, with (radio-quiet) Seyferts favoring spiral hosts whilst (radio-loud) Radio Galaxies are found exclusively in massive ellipticals, but the evidence for or against such a distinction for the ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node34.html -- 32.0 Кб -- 12.06.2006
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