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    • 1 | 2 | След.

    1. HST NICMOS Observations of Circumstellar Matter Around CYG X-3
    ... The morphology of the emission nebula can provide observational constraints for the predictions of the common envelope mass loss and the nebular emission can be used to place constraints on the initial mass of the system. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node24.html -- 32.3 Кб -- 12.06.2006
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    2. Unusual Emission near a Compact Source in Orion
    ... This was one of our motivations in obtaining high-resolution images of H 2 emission in the Orion Bar with NICMOS. ... The Orion Bar is the visible ionization boundary of the Orion Nebula, southeast of the Trapezium. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node23.html -- 19.0 Кб -- 12.06.2006
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    3. http://www.stecf.org/documents/isr/isr0102.pdf
    ... the spectrum of the Galactic Planetary Nebula NGC 7009, since the wealth of emission lines in their spectra makes Planetary ...
    [ Текст ]  Ссылки http://www.stecf.org/documents/isr/isr0102.pdf -- 222.9 Кб -- 11.05.2006
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    4. http://www.stecf.org/documents/isr/isr0603.pdf
    ... Based on the annular appearance of the emission lines (which are, effectively, monochromatic images of the nebula), the nebula itself is spatially resolved, while a spatially unresolved continuum from the central star is also seen. ...
    [ Текст ]  Ссылки http://www.stecf.org/documents/isr/isr0603.pdf -- 559.5 Кб -- 11.05.2006
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    5. IRAF/STECF 2-D spectrum point source / background decomposition package
    ... the right shows the intrinsic spectrum of the planetary nebula formed by subtracting the restored background image (top right ... Weak emission lines, such as [O III]4363A, are detectable. Hook, R.N., Lucy. L.B., Stockton, A. Ridgway, S., 1994. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/specres/ -- 16.5 Кб -- 08.06.2006
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    6. HST/NICMOS Observations of the Interacting System Arp 299
    ... as transition from pure H II region (such as the Orion Nebula) to an increasing r?le of shock excitation by supernova remnants ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node31.html -- 33.3 Кб -- 12.06.2006
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    7. ST-ECF IRAF package
    ... the right shows the intrinsic spectrum of the planetary nebula formed by subtracting the restored background image (top right ... Weak emission lines, such as [O III]4363A, are detectable. Hook, R.N., Lucy. L.B., Stockton, A. Ridgway, S., 1994. ...
    [ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/specres/index.php -- 19.0 Кб -- 09.04.2016
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    8. http://www.stecf.org/coordination/esa_eso/alma-herschel/report.pdf
    ... Figure 15: A sketch of the region close to the Kleinmann-Low nebula is shown. ... The shaded region in the NE to SW direction is the Ridge component, which is a part of very extended emission. ...
    [ Текст ]  Ссылки http://www.stecf.org/coordination/esa_eso/alma-herschel/report.pdf -- 1000.5 Кб -- 04.09.2008
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    9. http://www.stecf.org/documents/isr/WFC3-2009-17.pdf
    ... Sometimes the emission lines are affected by e.g., cosmic ray hits, hot/dead pixels etc. and thus good emission line centroids ...
    [ Текст ]  Ссылки http://www.stecf.org/documents/isr/WFC3-2009-17.pdf -- 1634.9 Кб -- 20.11.2009
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    10. http://www.stecf.org/documents/isr/isr0602.pdf
    ... of the SBC, the calibrator targets must exhibit strong emission lines with large equivalent widths in the wavelength range of ...
    [ Текст ]  Ссылки http://www.stecf.org/documents/isr/isr0602.pdf -- 416.5 Кб -- 11.05.2006
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