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    • [ В начало ] Пред. | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | След.

    91. http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_05_11_94
    ... 1.6 Completed WF/PC-2 5375 (High-Resolution Images of Virgo Galaxies with Kinematically Distinct Cores) The WF/PC-2 was used to make observations of galaxy NGC-4536 which is located in the Virgo Cluster. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_05_11_94 -- 4.4 Кб -- 12.05.1994
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    92. http://www.stsci.edu/~marel/abstracts/psdir/adiabat2.ps
    ... predict (at the distance of the Virgo cluster) that galaxies with M V < -21.2 have ... Profile shapes at the distance of the Virgo cluster Equations (4) and (7) predict r ...
    [ Текст ]  Ссылки http://www.stsci.edu/~marel/abstracts/psdir/adiabat2.ps -- 1453.2 Кб -- 02.11.1998
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    93. Galactic Flows: The Galaxy/IGM Ecosystem
    ... 1140: J. Kenney . Ram Pressure Stripping of Spiral Galaxies in the Virgo Cluster ( ppt ) . 1200: D. Rupke . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/igm/schedule -- 33.5 Кб -- 10.04.2016
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    94. http://www.stsci.edu/ftp/observing/status_reports/hst_status_05_29_02
    ... As a result, the distance to the Virgo cluster core remains uncertain by as much as 20 determination is directly affected by a lingering 0.1 mag {5 uncertainty in the photometric calibration of the WFPC2. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/hst_status_05_29_02 -- 11.8 Кб -- 30.05.2002
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    95. Colloquia - Spring 2005
    ... Feb., 26, 2005 . Patrick Cote, HIA, National Research Council Canada . The ACS Virgo Cluster Survey . Jan., 05, 2005 . No Colloquium . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/smo/events/colloquia/2005-spring -- 19.2 Кб -- 11.04.2016
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    96. http://www.stsci.edu/ftp/observing/status_reports/hst_status_05_16_02
    ... As a result, the distance to the Virgo cluster core remains uncertain by as much as 20 determination is directly affected by a lingering 0.1 mag {5 uncertainty in the photometric calibration of the WFPC2. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/hst_status_05_16_02 -- 7.3 Кб -- 17.05.2002
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    97. http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-STScI-000383.pdf
    ... pushes this requirement the hardest is Microlensing in the Virgo Cluster, which is aiming for precise relative photometry of ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-STScI-000383.pdf -- 205.8 Кб -- 05.02.2013
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    98. http://www.stsci.edu/~marel/abstracts/psdir/lauer4.ps
    ... with # # 1 into the HST resolution limit; for galaxies in the Virgo cluster this corresponds to radii of only a few parsecs ... NGC 3706 thus appears to be a core galaxy. 2.3. NGC 4406 NGC 4406 is a giant elliptical galaxy in the Virgo cluster. ...
    [ Текст ]  Ссылки http://www.stsci.edu/~marel/abstracts/psdir/lauer4.ps -- 2580.5 Кб -- 14.06.2002
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    99. http://www.stsci.edu/~marel/abstracts/psdir/2002AJ....124.1975L.ps
    ... with # # 1 into the HST resolution limit; for galaxies in the Virgo Cluster this corresponds to radii of only a few parsecs ... NGC 3706 thus appears to be a core galaxy. 2.3. NGC 4406 NGC 4406 is a giant elliptical galaxy in the Virgo Cluster. ...
    [ Текст ]  Ссылки http://www.stsci.edu/~marel/abstracts/psdir/2002AJ....124.1975L.ps -- 1568.3 Кб -- 29.11.2002
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    100. http://www.stsci.edu/ftp/observing/status_reports/hst_status_05_27_02
    ... As a result, the distance to the Virgo cluster core remains uncertain by as much as 20 determination is directly affected by a lingering 0.1 mag {5 uncertainty in the photometric calibration of the WFPC2. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/hst_status_05_27_02 -- 16.1 Кб -- 28.05.2002
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