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    1. HST/NICMOS Observations of the Interacting System Arp 299
    ... is one of the nearest examples of interacting galaxies with a high infrared (IR ... in the interacting system are derived. galaxies, interacting, stellar content, star ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node31.html -- 33.3 Кб -- 12.06.2006
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    2. NICMOS Imaging of QSO Host Galaxies at 0.1 < z < 4.4
    ... Of the six objects for which data have been obtained the results range from no host galaxy detected, to an obvious galaxy with an interacting companion, to a possible high redshift galaxy cluster. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node35.html -- 5.1 Кб -- 12.06.2006
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    3. Robust, Realtime Bandpass Removal for the HI Parkes All Sky Survey Project
    ... Figure 1: Raw (top) and calibrated flux densities for a selected channel of a HIPASS scan through the interacting galaxy ESO 269-IG 056 (cycles 34-41) and the continuum source PKS 1307-403 (cycles 66-73)-- see text . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/barnesd2.html -- 14.4 Кб -- 12.06.2006
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    4. http://www.stecf.org/conferences/adass/adassVII/reprints/barnesd2.pdf
    ... Raw (top) and calibrated flux densities for a selected channel of a HIPASS scan through the interacting galaxy ESO 269-IG 056 (cycles 34­41) and the continuum source PKS 1307-403 (cycles 66­ 73)--see text. ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/barnesd2.pdf -- 141.9 Кб -- 12.06.2006
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    5. http://www.stecf.org/conferences/adass/adassVII/reprints/barnesd2.ps.gz
    ... Raw (top) and calibrated flux densities for a selected chan­ nel of a HIPASS scan through the interacting galaxy ESO 269­IG 056 (cycles 34--41) and the continuum source PKS 1307­403 (cycles 66-- 73)---see text. ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/barnesd2.ps.gz -- 113.4 Кб -- 12.06.2006
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    6. http://www.stecf.org/coordination/esa_eso/alma-herschel/report.pdf
    ... The study of interacting galaxies will improve our knowledge of star formation triggered 28 by interactions. ... 2005). This is a well-known group of interacting galaxies and has some 40 members representing all morphological types. ...
    [ Текст ]  Ссылки http://www.stecf.org/coordination/esa_eso/alma-herschel/report.pdf -- 1000.5 Кб -- 04.09.2008
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    7. http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/szokoly04.ps
    ... X-ray type-1 QSO/AGN (XID 30, 101), X-ray type-2 QSO/AGN (XID 56, 201, 263), and interacting galaxy pairs (XID 98, 138, 580 ... three HEX objects are X-ray galaxies (XID 98a, 175b, 580a), two being members of interacting pairs, and all have HR = 1:0 ...
    [ Текст ]  Ссылки http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/szokoly04.ps -- 1186.7 Кб -- 16.09.2004
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    8. A Color Analysis of NICMOS Parallel Observations
    ... In addition to the aforementioned blank fields and blurred images, we have noticed few galaxies relative to point sources, and among these several interacting systems, which are likely to be infrared-luminous. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node28.html -- 19.5 Кб -- 12.06.2006
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    9. NICMOS Science
    ... HST-NICMOS Observations of Galactic Bulges: Red Nuclei in Nearby Galaxies . ... HST /NICMOS Observations of the Interacting System Arp 299 . Introduction . ... Object Sizes . Implications of the Galaxy Counts . Extremely Red Objects . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node18.html -- 15.2 Кб -- 12.06.2006
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    10. The Evolution of Stars seen with ISOCAM - the Need for NICMOS and VLT Follow...
    ... The targets of ISO had been all over in the Universe: in the Solar System, towards Comets and the Zodiacal Light, Giant Molecular Clouds, Protoplanetary Disks, the Galaxy and still further away to Interacting Systems and QSO in distant Cluster. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node22.html -- 26.3 Кб -- 12.06.2006
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