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    51. http://www.stecf.org/conferences/adass/adassVII/reprints/prukschm.pdf
    ... The star in the upper right is ten times brighter than the weakest star in the cluster and allows to determine the point-spread function. 1 http://www.jpl.nasa.gov/galileo/messenger/oldmess/Ida2.gif 498 Pruksch and Fleischmann Figure 2. ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/prukschm.pdf -- 112.2 Кб -- 12.06.2006
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    52. The Co-Addition Technique Applied to Images of Galaxy Cores
    ... is attributed to tidal stripping of a star during a close encounter with a central ... Assuming the complete disruption of the star, the flare is expected to be visible ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/zeilingerw.html -- 10.8 Кб -- 12.06.2006
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    53. The VizieR System for Accessing Astronomical Data
    ... source=I/239/hip_main&HIP=12345 ; or a pointer to all Tycho stars closer than to Sirius, ordered by their increasing distance to the brightest star, can be written by a call to VizieR with parameters: 1>0 . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/ochsenbeinf.html -- 16.5 Кб -- 12.06.2006
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    54. http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.pdf
    ... is attributed to tidal stripping of a star during a close encounter with a central ... Assuming the complete disruption of the star, the flare is expected to be visible ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.pdf -- 49.4 Кб -- 12.06.2006
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    55. A Color Analysis of NICMOS Parallel Observations
    ... limit of these observations should also allow the detection of the recently discovered population of young ( 1 Gyr) star-forming galaxies at z 3 (Steidel et al. 1996), based on their K-band fluxes, as well as star-forming galaxies at lower redshifts ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node28.html -- 19.5 Кб -- 12.06.2006
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    56. http://www.stecf.org/conferences/adass/adassVII/reprints/llebariaa.pdf
    ... error signal is taken from an independent star tracker centered on a guide star (using the visible part of its spectrum ... for: 1) Stars from an uncorrected image, 2) Stars from a corrected image using a reference (see algorithm 1), 3) Stars from a ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/llebariaa.pdf -- 126.9 Кб -- 12.06.2006
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    57. http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.ps.gz
    ... is attributed to tidal stripping of a star during a close encounter with a central ... Assuming the complete disruption of the star, the flare is expected to be visible ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/zeilingerw.ps.gz -- 76.9 Кб -- 12.06.2006
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    58. HST NICMOS Observations of Circumstellar Matter Around CYG X-3
    ... binaries: close - stars: individual: Cyg X-3 - stars: Wolf-Rayet - infrared: stars ... star that can be used to make the AO wavefront corrections is 30 away from Cyg X-3 ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node24.html -- 32.3 Кб -- 12.06.2006
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    59. Parallel Tree N-body Code: Data Distribution and DLB on the CRAY T3D for Large
    ... Next: Modelling Spectro-photometric Characteristics of Nonradially Pulsating Stars . Up: Computational Astrophysics . ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/beccianiu.html -- 16.7 Кб -- 12.06.2006
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    60. http://www.stecf.org/conferences/adass/adassVII/reprints/llebariaa.ps.gz
    ... error signal is taken from an independent star tracker centered on a guide star (using the visible part of its spectrum ... for: 1) Stars from an uncorrected image, 2) Stars from a corrected image using a reference (see algorithm 1), 3) Stars from a ...
    [ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/llebariaa.ps.gz -- 97.2 Кб -- 12.06.2006
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