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    • [ В начало ] Пред. | 11 | 12 | 13 | 14 | 15 | 16 | 17 | 18 | 19 | 20 | След.

    141. Star-Forming or Starbursting? The Ultraviolet Conundrum
    ... dust geometries and dust extinction curves are the most likely causes for the observed dispersion in the IRX-ЮВ diagram, (3) together with some potential dilution of the most recent star-forming population by older unrelated bursts, at least in the case ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2009ApJ...706..553B.html -- 4.5 Кб -- 21.01.2016
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    142. http://www.stsci.edu/hst/stis/documents/isrs/199904.pdf
    ... STIS Instrument Science Report 99-04 DUST MOTES AND BLEMISHES IN THE CCD SPECTRAL MODES Ralph Bohlin July 1999 ABSTRACT A set of 84 dust mote features and blemishes have been identified in STIS CCD flat fields. ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/stis/documents/isrs/199904.pdf -- 369.9 Кб -- 07.12.2004
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    143. ST ScI Preprint #1367
    ... complementing the restframe UV data; they offer a better handle on the amount of dust obscuration present in the galaxies, although some ambiguity remains as to the distribution of the dust withing the system and the opacit correction factor this implies ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1367/prep1367.html -- 4.2 Кб -- 29.11.2000
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    144. Less Common Common Dust Features in Evolved Stars
    ... dust temperature is something like 150 K. The star seems to have stopped producing ... dust shell models suggest that this transition in temperatures takes some period of ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~volk/features2.html -- 13.9 Кб -- 27.05.2014
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    145. http://www.stsci.edu/stsci/meetings/planets/abs/prog2.html
    ... When operated 5 AU from the Sun to escape background emission from local zodiacal dust, the interferometer's sensitivity will be fundamentally limited by noise in the photon flux from warm zodiacal dust in the planetary system under observation. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/planets/abs/prog2.html -- 3.8 Кб -- 22.10.1996
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    146. Extended Mid-Infrared Aromatic Feature Emission in M82
    ... We also see significant emission by dust well outside the superwind region, providing the clearest picture to date of the dust distribution in the halo of this galaxy. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2006ApJ...642L.127E.html -- 4.3 Кб -- 21.01.2016
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    147. Surveying the Agents of Galaxy Evolution in the Tidally Stripped, Low
    ... A preliminary estimate of the dust production in AGB and RSG stars reveals that the extreme C-rich AGB stars dominate the dust input in both galaxies, and that the O-rich stars may play a larger role in the LMC than in the SMC. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2011AJ....142..103B.html -- 5.1 Кб -- 21.01.2016
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    148. Detection of Extended Red Emission in the Diffuse Interstellar Medium
    ... or if it is an observational feature of all dust, i.e., present in the diffuse ... that they were taken outside the zodiacal dust cloud and, therefore, are free from ... were entirely caused by scattering from dust (i.e., diffuse Galactic light or DGL ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/1998ApJ...498..522G.html -- 5.2 Кб -- 21.01.2016
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    149. Marshall Perrin's Research
    ... high contrast: scattered light from circumstellar dust is faint, usually less than a ... starlight can completely swamp the dust-scattered light and prevent detection ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~mperrin/research.shtml -- 15.4 Кб -- 10.04.2016
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    150. Silicon Nanoparticles: Source of Extended Red Emission?
    ... About 36% of the interstellar silicon that is depleted into the dust phase would be needed in the form of silicon nanoparticles, amounting to less than 5% of the interstellar dust mass. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/1998ApJ...501L.111W.html -- 4.5 Кб -- 21.01.2016
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    [ В начало ] Пред. | 11 | 12 | 13 | 14 | 15 | 16 | 17 | 18 | 19 | 20 | След.

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