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    1. Superluminal Motion in the M87 Jet
    ... Superluminal Motion in the M87 Jet. ... TOP PANEL: Hubble image showing jet streaming out from the galaxy's nucleus [bright round region at far left]. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/science/m87/m87.html -- 8.6 Кб -- 08.01.1999
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    2. STScI Preprint #1328
    ... jet, except in the "shock-like" knot regions (parts of HST-1, A, and C), where it ... in the inner jet, giving us important insight into the radial structure of the jet ... jet interior, where higher-energy electrons are concentrated and dominate both ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1328/prep1328.html -- 5.4 Кб -- 14.07.2000
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    3. STScI Preprint #1335
    ... jet, with eight of these having apparent speeds in the range 4c to 6c. Two additional features within the first arcsecond of ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1335/prep1335.html -- 4.7 Кб -- 14.07.2000
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    4. http://www.stsci.edu/stsci/meetings/planets/abs/prog23.html
    ... Jet Propulsion Laboratory, California Institute of Technology, Pasadena CA . ... DG Tau shows a number of arcs of reflection nebulosity and significant jet structure ... DG Tau B has a thick absorbing disk with a bipolar jet. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/planets/abs/prog23.html -- 3.7 Кб -- 22.10.1996
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    5. ST ScI Preprint #1383
    ... To do so, we make the assumptions that the inner radio jet is perpendicular to the X-ray observed inner accretion disk, and that the observed jet (or the stronger component, if the jet is two-sided) is physically closer to Earth than the plane of the ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1383/prep1383.html -- 5.1 Кб -- 25.01.2001
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    6. STScI Preprint #1271
    ... in the shock-like knots A and C. We also find considerable evidence for structure in the jet as a function of distance from the jet axis - evidence is seen for radial structure in the radio / optical spectrum, in the optical / optical spectrum, and in the ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1271/prep1271.html -- 6.6 Кб -- 23.05.2000
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    7. HST this week
    ... GO 10762: The long X-ray jet of Quasar 4C19.44. ... Abstract . 10603 . Deborah Padgett, Jet Propulsion Laboratory . ... The Long X-ray Jet of Quasar 4C19.44 . Abstract . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/thisweek1/thisweek79.html -- 12.3 Кб -- 08.06.2007
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    8. STScI Preprint #1215
    ... Because the electron density is substantially larger in the jet compared to the surrounding NLR, these results can only be explained if there is a more intense ionizing continuum associated with the jet. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1215/prep1215.html -- 7.0 Кб -- 23.05.2000
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    9. STScI Preprint #1224
    ... we ask if this apparent absence of "jet lines" in the spectra of most CVs already implies the absence of jets of the kind that appear to be present in the SSSs and perhaps T Pyx, or whether the current lack of jet detections in CVs can still be ascribed ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1224/prep1224.html -- 5.8 Кб -- 23.05.2000
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    10. http://www.stsci.edu/ftp/stsci/library/abstracts/1126.abs
    ... jet collimation, brightness, and orientation change dramatically as it crosses the ... model for the jet propagation in which an initially relativistic jet decelerates as ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/stsci/library/abstracts/1126.abs -- 4.0 Кб -- 06.03.1997
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