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    1. HST Spectral Maps of Accretion Disks in Cataclysmic Binaries
    ... eclipse mapping techniques are used in the analysis of HST/FOS time-resolved low ... Figure: (a) Average out-of-eclipse (dark) and mid-eclipse (light) spectra of UX UMa ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/baptistar.html -- 12.0 Кб -- 15.06.2005
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    2. Eclipse Decomposition of Time-Resolved UBVRI and HST Spectra of the Dwarf Nova
    ... Eclipse Decomposition of Time-Resolved UBVRI and HST Spectra of the Dwarf Nova IP Peg . Abstract: . Introduction . ... developed by Keith Horne and Tom Marsh and its application on HST-data of the eclipsing dwarf nova IP Peg will be presented ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/wolfs.html -- 12.5 Кб -- 15.06.2005
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    3. STScI Preprint #1204
    ... This is clear from the plethora of emission lines that appear in the mid-eclipse spectra, some of which appear as absorption features in spectra taken at out-of-eclipse orbital phases. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1204/prep1204.html -- 7.5 Кб -- 23.05.2000
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    4. STScI Preprint #1207
    ... Their amplitudes are highest at pre-eclipse orbital phases and exhibit a rather gradual eclipse whose shape is roughly similar to, though perhaps slightly narrower than, UX UMa's overall light curve in the PRISM bandpass (2000 - 8000 ). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1207/prep1207.html -- 8.1 Кб -- 23.05.2000
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    5. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_10_18_95
    ... FOS/RD 6089 (Eclipse Mapping and Tomography of the UV = Emitting Region of DQ Her) The Faint Object Spectrograph (Red Side) was used to make rapid = mode ultraviolet observations of the eclipsing binary star DQ-Her in order = to do eclipse mapping and ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_10_18_95 -- 4.4 Кб -- 18.10.1995
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    6. The Spectroscopic Orbit of the Evolved Binary HD 197770
    ... taken between 1992 and 1997 to derive the spectroscopic orbit of the eclipsing double-lined spectroscopic binary HD 197770 ... for A and B are 2.9 and 1.9, respectively, and are close to the actual masses because of the eclipsing nature of this binary ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/1998AJ....115.2561G.html -- 4.1 Кб -- 21.01.2016
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    7. Home Page of Kailash Sahu
    ... Recently, my research has been mainly focused on a large HST program called SWEEPS (Sagittarius Window Eclipsing Extrasolar Planet Search). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~ksahu/ -- 5.1 Кб -- 23.12.2015
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    8. http://www.stsci.edu/science/preprints/prep1207/prep1207.bib
    ... Their amplitudes are highest at pre-eclipse orbital phases and exhibit a rather gradual eclipse whose shape is roughly similar to, though perhaps slightly narrower than, UX UMa's overall light curve in the PRISM bandpass (2000 Å&nbsp ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1207/prep1207.bib -- 5.6 Кб -- 07.10.1998
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    9. http://www.stsci.edu/science/preprints/prep1204/prep1204.bib
    ... This is clear from the plethora of emission lines that appear in the mid-eclipse spectra, some of which appear as absorption features in spectra taken at out-of-eclipse orbital phases. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1204/prep1204.bib -- 5.0 Кб -- 07.10.1998
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    10. John H. Debes
    ... 9.24.2012 The WIRED Survey III: An Infrared Excess around the Eclipsing Post-Common Envelope Binary SDSS J030308.35+005443.7 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~debes/newsarchive.html -- 16.2 Кб -- 27.09.2012
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