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    51. Ultraviolet through Far-Infrared Spatially Resolved Analysis of the Recent Star
    ... Ultraviolet through Far-Infrared Spatially Resolved Analysis of the Recent Star Formation in M81 (NGC 3031) . ... from IR monochromatic fluxes, and we compare five different star formation rate (SFR) estimators for H II regions in M81 and ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2006ApJ...648..987P.html -- 5.2 Кб -- 21.01.2016
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    52. Spitzer SAGE Infrared Photometry of Massive Stars in the Large Magellanic Cloud
    ... Spitzer SAGE Infrared Photometry of Massive Stars in the Large Magellanic Cloud . ... We find the infrared colors for Wolf-Rayet stars to be independent of spectral type and their SEDs to be flatter than what ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2009AJ....138.1003B.html -- 4.9 Кб -- 21.01.2016
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    53. WFPC2 Bright Star Avoidance Regions
    ... 2) Providing rudimentary estimates for magnitudes of stars in the field, which is useful when planning exposures, e.g., to avoid bright stars near WFPC2 which may result in scattered light. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/wfpc2/analysis/avoid.html -- 16.5 Кб -- 10.04.2016
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    54. Low-mass Companions to Nearby Stars
    ... Space Telescope Science Institute . Low-mass Companions to Nearby Stars . Low-mass Companions to Nearby Stars . Todd Henry . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/planets/prog9.html -- 9.4 Кб -- 10.04.2016
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    55. WFPC2 Instrument Handbook Update
    ... rates observed for the same star (i.e., throughput ratio) as a function of the change in Y position for stars in 4 different ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instrument-news/handbooks/wfpc2/98update/update0698.fm1.html -- 6.8 Кб -- 23.06.1998
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    56. Infrared Imaging of the Large Magellanic Cloud Star-forming Region Henize 206
    ... As is also seen in early Spitzer observations of M81, star formation rates calculated from HЮБ for Henize 206 may miss the deeply embedded young stars, compared with star formation rates calculated from far infrared emission. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2004ApJS..154..275G.html -- 4.3 Кб -- 21.01.2016
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    57. The Calibration of Mid-Infrared Star Formation Rate Indicators
    ... The Calibration of Mid-Infrared Star Formation Rate Indicators . ... SFR, we analyze Spitzer 8 and 24 ЮМm data of star-forming regions in a sample of 33 nearby galaxies with available HST NICMOS ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2007ApJ...666..870C.html -- 5.5 Кб -- 21.01.2016
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    58. How often would I have to acquire new guide stars?
    ... Hubble Space Telescope . How often would I have to acquire new guide stars?. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/nicmos/faqs/guidestars.faq -- 17.2 Кб -- 10.04.2016
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    59. Spitzer Sage Survey of the Large Magellanic Cloud. III. Star Formation and
    ... Spitzer Sage Survey of the Large Magellanic Cloud. III. Star Formation and ~1000 New Candidate Young Stellar Objects . ... to high-mass and young evolutionary stages, because these overlap less with galaxies and evolved stars in color-magnitude space ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2008AJ....136...18W.html -- 5.9 Кб -- 21.01.2016
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    60. Howard E. Bond--Effects, Stars, and Discoveries
    ... Bull. on Var. Stars No. 1160 . The star is now named "Bond's Flare Star" or AF Psc, and its spectrum was subsequently analyzed by Jesse Greenstein . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~bond/effects.html -- 5.3 Кб -- 20.10.2001
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