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    • 1 | 2 | След.

    1. http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/cristiani00.pdf
    ... In the AXAF field two relatively close pairs of galaxies have been identified, with separations of 8.7 and 3.1 proper Mpc and ... It is interesting to note that two relatively close pairs of galaxies are observed in the AXAF field. ...
    [ Текст ]  Ссылки http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/cristiani00.pdf -- 221.3 Кб -- 16.09.2004
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    2. HST/NICMOS Observations of the Interacting System Arp 299
    ... Following the notation introduced by Gehrz et al. (1983) for the interacting pair of galaxies Arp 299, the nucleus of IC 694 (eastern component) is referred to as source A, and the sources in NGC 3690 (western component) are called B1, B2, C and C (see ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node31.html -- 33.3 Кб -- 12.06.2006
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    3. http://www.stecf.org/coordination/esa_eso/cosmology/report.pdf
    ... amplitude also depends on the apparent angular separation between galaxy pairs ... by overlapping galaxies Very close galaxy pairs have overlapping isophotes that ... be corrected by a judicious weighting of galaxy pairs as function of their redshift ...
    [ Текст ]  Ссылки http://www.stecf.org/coordination/esa_eso/cosmology/report.pdf -- 1894.6 Кб -- 04.09.2008
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    4. Robust, Realtime Bandpass Removal for the HI Parkes All Sky Survey Project
    ... Previous: The Co-Addition Technique Applied to Images of Galaxy Cores . ... For a given beam and polarization pair, the target spectrum is , and the reference ... the parent matrix select a beam-polarization pair, and the row and column in the sub ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/barnesd2.html -- 14.4 Кб -- 12.06.2006
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    5. 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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    6. http://www.stecf.org/documents/isr/ISR_NGST_2002-03.pdf
    ... The expected number of galaxies in this region is r , where is the number density of objects (galaxies/degree2) derived from ...
    [ Текст ]  Ссылки http://www.stecf.org/documents/isr/ISR_NGST_2002-03.pdf -- 748.2 Кб -- 11.05.2006
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    7. http://www.stecf.org/conferences/adass/adassVII/reprints/barnesd2.pdf
    ... For a given beam and polarization pair, the target spectrum is Ib,p,ctarget , and ... the parent matrix select a beam-polarization pair, and the row and column in the sub ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/barnesd2.pdf -- 141.9 Кб -- 12.06.2006
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    8. http://www.stecf.org/conferences/adass/adassVII/reprints/barnesd2.ps.gz
    ... For a given beam and polarization pair, the target spectrum is I b,p,ctarget , and ... in the parent matrix select a beam­polarization pair, and the row and column in the ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/barnesd2.ps.gz -- 113.4 Кб -- 12.06.2006
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    9. http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/croom01.pdf
    ... However, the large angular separation makes this pair an unlikely candidate for a gravitational lens. ... The remaining identifications are all galaxies, with roughly equal numbers of early- and late-type spectra (by early and late ...
    [ Текст ]  Ссылки http://www.stecf.org/goods/spectroscopy/CDFS_Mastercat/croom01.pdf -- 588.2 Кб -- 16.09.2004
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    10. The Formation and Evolution of LMC Rich Star Clusters: NGC 1818
    ... origin and evolution of rich star clusters in our own Galaxy, in the LMC, and beyond ... These are grouped into four age pairs, with ages of 10 7 -10 10 yr. ... Again, it is possible that these are field stars and/or background galaxies. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node27.html -- 15.4 Кб -- 12.06.2006
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