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    51. http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_07_14_97
    ... as planned, and no problems were reported 1.22 Completed WF/PC-2 6737 (Imaging Reflection Nebulosity in Three Post-AGB Objects) The WF/PC-2 was used to make observations of the reflection nebula surrounding the post-AGB objects HD179821 and HD161796 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_07_14_97 -- 15.5 Кб -- 14.07.1997
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    52. http://www.stsci.edu/~golim/papers/krist2005b.pdf
    ... from circumstellar material, an asymmetrical distribution of light about the line of sight on the near edge of the disk, enhanced brightness along the near edge of the disk due to forward scattering, and a compact reflection nebula near the secondary star ...
    [ Текст ]  Ссылки http://www.stsci.edu/~golim/papers/krist2005b.pdf -- 345.1 Кб -- 01.12.2005
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    53. http://www.stsci.edu/ftp/instrument_news/FOC/Foc_isr/foc_isr069.ps
    ... H.­M. Adorf, P. Benvenuti, A. Caulet, R. Fosbury, R. Hook 1 Introduction Previous observations for calibration of the FOC polarizers (proposals 1521 and 3873) have been of polarized, nebulous objects, the jet of M 87 and the reflection nebula Lick Hff 233 ...
    [ Текст ]  Ссылки http://www.stsci.edu/ftp/instrument_news/FOC/Foc_isr/foc_isr069.ps -- 80.0 Кб -- 04.10.1994
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    54. http://www.stsci.edu/institute/org/ins/files/DMMReports/2004DMMReports/Dec2004
    ... Program 10378 will observe a highly polarized reflection nebula to check for phase retardance effects in ACS polarimetry. ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/org/ins/files/DMMReports/2004DMMReports/Dec2004 -- 383.5 Кб -- 10.01.2005
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    55. Poster Abstracts
    ... This has already been done for Extended Red Emission, which is an optical emission feature of dust, using HST ACS NICMOS imaging of narrow filaments in the reflection nebula NGC 7023 (Witt et al. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/jwst2007/posterAbstracts.html -- 86.8 Кб -- 11.04.2016
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    56. http://www.stsci.edu/hst/wfpc2/documents/isr/wfpc2_isr9507.pdf
    ... To establish the zeropoint of the polarizer orientation it is necessary to observe a highly polarized source; a reflection nebula was chosen for its large size and 10-20% polarization. ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfpc2/documents/isr/wfpc2_isr9507.pdf -- 453.3 Кб -- 05.02.2013
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    57. http://www.stsci.edu/hst/wfpc2/documents/isr/wfpc2_isr9702.pdf
    ... 2/3/97 WFPC2 Cycle 5 Calibration Closure Report Page 34 (A) 12 10 8 ARC SEC 6 4 2 0 -2 (B) -10 -5 ARC SEC 0 5 Figure 9: WFPC2 polarimetric images of the reflection nebula surrounding R Mon from calibration proposal 5574. ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfpc2/documents/isr/wfpc2_isr9702.pdf -- 534.9 Кб -- 05.02.2013
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    58. http://www.stsci.edu/~INS/2010CalWorkshop/carey.pdf
    ... To quantify this effect, the IRAC instrument supp ort team conducted measurements of HI I regions and bright reflection nebula previously imaged by MSX at 8.3 µm and with good quality ISO SWS sp ectra to provide SED information. ...
    [ Текст ]  Ссылки http://www.stsci.edu/~INS/2010CalWorkshop/carey.pdf -- 659.8 Кб -- 23.04.2012
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    59. http://www.stsci.edu/~webdocs/STScINewsletter/1995/october95.pdf
    ... 939. "Scattering Properties of the Dust in the Reflection Nebula IC 435" D. Calzetti, R.C. Bohlin, K.D. Gordon, A.N. Witt, L. Bianchi. 940. ...
    [ Текст ]  Ссылки http://www.stsci.edu/~webdocs/STScINewsletter/1995/october95.pdf -- 444.4 Кб -- 19.01.2009
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    60. http://www.stsci.edu/~robberto/Main/Recent%20papers/ApJ129.1534.pdf
    ... Werner et al. (1983) were the first to report that at 4.8 m the BN / KL complex is predominantly a reflection nebula, but since the albedo of astronomical silicates drops by 2 orders of magnitude between No. ...
    [ Текст ]  Ссылки http://www.stsci.edu/~robberto/Main/Recent%20papers/ApJ129.1534.pdf -- 1795.0 Кб -- 13.01.2006
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