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    1. Molecular hydrogen emission in the interstellar medium of the Large Magellanic
    ... Molecular hydrogen emission in the interstellar medium of the Large Magellanic Cloud . ... We present the detection and analysis of molecular hydrogen emission towards ten interstellar regions in the Large Magellanic ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2015MNRAS.446.2490N.html -- 4.8 Кб -- 21.01.2016
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    2. An Extremely Large Excess of 18O in the Hydrogen-deficient Carbon Star HD...
    ... An Extremely Large Excess of 18O in the Hydrogen-deficient Carbon Star HD 137613 . ... discovery of a uniquely large excess of 18O in the hydrogen-deficient carbon (HdC) star HD 137613 based on a spectrum of the ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2005ApJ...623L.141C.html -- 4.4 Кб -- 21.01.2016
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    3. SINGG: The HIPASS H-alpha survey
    ... The HIPASS H-alpha survey is a project to measure ionized hydrogen in a sample of 500 galaxies selected via their 21-cm neutral hydrogen emission. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/science/singg/ -- 5.1 Кб -- 08.09.2003
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    4. http://www.stsci.edu/instrument-news/handbooks/nicmos/c11_reference.doc6.html
    ... Infrared Line Lists . Table 12.9: Recombination Lines of Atomic Hydrogen: Paschen Series 1 . Transition . (Nu - Nl) . ... cm -1) . I/I(Hbeta) . Te=Ne=104 . Table 12.10: Recombination Lines of Atomic Hydrogen: Brackett Series . Transition . (Nu-Nl) . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instrument-news/handbooks/nicmos/c11_reference.doc6.html -- 38.2 Кб -- 07.08.1997
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    5. John H. Debes
    ... Often, they have a thin atmosphere of helium or hydrogen. Any element heavier than helium. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~debes/dust.html -- 10.5 Кб -- 23.11.2011
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    6. All kinds of death - 12
    ... Sun is powered by nuclear fusion: hydrogen `burns' to form helium, releasing energy ... but the supply of hydrogen is not infinite. ~10% of the Sun's mass is available as ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/observ/dpics/d12.htm -- 6.0 Кб -- 08.06.2007
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    7. STScI Preprint #1250
    ... An Arecibo Search for Broad 21 cm Lines of Atomic Hydrogen in Clusters of Galaxies. ... which is allowed by the observations makes it unlikely that there is very much atomic hydrogen in the ICM of these clusters ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1250/prep1250.html -- 5.6 Кб -- 23.05.2000
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    8. Spectroscopy of Planetary Nebulae
    ... Simulated Pure Hydrogen Spectrum . Simulated Hydrogen and Helium Only Spectrum. ... Simulated Pure Hydrogen Spectrum . Simulated Hydrogen and Helium Only Spectrum. ... here could be identified as due to Hydrogen and Helium, while many of the other ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~volk/pnspectra.html -- 9.4 Кб -- 21.04.2011
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    9. STScI Preprint #1237
    ... The hydrogen component in a highly inhomogeneous universe is completely reionized when the number of ionizing photons emitted in one recombination time equals the mean number of hydrogen atoms. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1237/prep1237.html -- 5.1 Кб -- 23.05.2000
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    10. Analysis of in B-Type Stars
    ... The hydrogen line is the most pronounced absorption feature in spectra of B-type ... Theoretical profiles of the hydrogen line are calculated for Kurucz's (1979) models ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/nowakd.html -- 18.5 Кб -- 15.06.2005
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