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    41. http://www.atnf.csiro.au/people/bkoribal/publications/S217_EngKor.ps
    ... NGC 3256 appears to have 10 00 diameter ux density enhancements in its tidal tails and in its detached gas fragments. ... NGC 3263 displays a 30 kpc long tidal tail which has a perpendicular extension devoid of stars. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/bkoribal/publications/S217_EngKor.ps -- 486.8 Кб -- 16.10.2003
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    42. http://www.atnf.csiro.au/research/pulsar/ppta-obs/dashboard/docs/ppta_obsstrategy_rms.pdf
    ... tails · If pulsar is bright, stays bright for some Dme (hours) · If pulsar is faint, remains faint for a similar length · Results in large variaDons in TOA uncertainty · Non- detecDons (5- sigma) detecDons are worthless · ScinDllaDon can change the gain ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/pulsar/ppta-obs/dashboard/docs/ppta_obsstrategy_rms.pdf -- 418.6 Кб -- 04.12.2015
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    43. http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/proceedings/SEA_Barcelona_2006_lopez-sanchez.pdf
    ... cases. (merger remants, arcs, ripples, tails, tidal dwarf galaxies) with external ... diagram for the slit a tidal tail is clearly detected. and the kinematics of the ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/proceedings/SEA_Barcelona_2006_lopez-sanchez.pdf -- 394.2 Кб -- 30.10.2006
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    44. Uncovered Structures and the Cluster Abell 3627
    ... the ROSAT PSPC observations; the right panel shows the residual X-ray contours after substraction of a spherical component, and the 843 MHz radio continuum emission of the wide-angle tail radio galaxy PKS1610-60.8 and the head-tail radio-source B1610-60.5 ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_1/renee/paper/node4.html -- 57.5 Кб -- 08.04.2016
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    45. http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/posters/Mexico2002.pdf
    ... features, like mergers or tidal tails connecting small stellar aggregates, are found ... found several faint objects connected by bridges and tails with the main body of the ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/posters/Mexico2002.pdf -- 733.0 Кб -- 03.02.2008
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    46. http://www.atnf.csiro.au/research/mag_stream/bruens.ps.gz
    ... Head-tail structures The high velocity resolution (v = 0.8 km s 1 ) of this HI survey allows a de- tailed analysis of the shape of individual line-pro les. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/mag_stream/bruens.ps.gz -- 264.4 Кб -- 31.07.2000
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    47. Results
    ... For models with , the high-tail of the distribution function rarely extends beyond 4'', while for models, the high-tail often extends to separations of 6''. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/18_2/premadi/paper/node4.html -- 68.0 Кб -- 08.04.2016
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    48. http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/posters/IAU217_australia2003.pdf
    ... P.A. 128є, figure 3c) and an optical tidal tail that seems to be extending from the ... F1 and F2 seem clearly to be kinematically different of this optical tidal tail. ... et al. 1991) and the optical tidal tail (blue-violet contour, Iglesias-PАramo ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/posters/IAU217_australia2003.pdf -- 495.8 Кб -- 03.02.2008
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    49. http://www.atnf.csiro.au/research/Astro2010/talks/ferrario.pdf
    ... A high magnetic field tail in HFMWDs. Contribution from mergers? ... WDs · Most MWDs have massive(>3M) progenitors A high mass tail with clear contribution from mergers · BUT many massive WDs are ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/Astro2010/talks/ferrario.pdf -- 1130.3 Кб -- 16.06.2010
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    50. http://www.atnf.csiro.au/people/Ray.Norris/papers/n272.pdf
    ... 4.3 Tailed radio galaxies Tailed radio galaxies are found in large clusters, and are ... tailed galaxies in ATLAS, from which they estimate between 26 в 103 and 2 в 105 ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Ray.Norris/papers/n272.pdf -- 317.6 Кб -- 21.04.2011
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