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    1. 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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    2. 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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    3. Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for
    ... It is by no means exhaustive. Table B.9: Recombination Lines of Atomic Hydrogen: Paschen Series . Transition . (N u - N l ) . ... Table B.10: Recombination Lines of Atomic Hydrogen: Brackett Series. Transition . (N u -N l ) . Vacuum Wavelength . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/nicmos/documents/handbooks/current_NEW/Appendix_B.14.6.html -- 330.1 Кб -- 05.02.2013
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    4. Herschel Exploitation of Local Galaxy Andromeda (HELGA). III. The Star
    ... Atomic hydrogen (H I) and molecular gas (traced by carbon monoxide, CO) or the dust mass is used to trace the total gas in the ISM. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2013ApJ...769...55F.html -- 5.0 Кб -- 21.01.2016
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    5. Physical Conditions in the Ionized Gas of 30 Doradus
    ... Aromatic dust emission features and emission lines from molecular and atomic hydrogen are detected but they are not particularly strong. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2009ApJ...694...84I.html -- 4.5 Кб -- 21.01.2016
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    6. http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_09_08_95
    ... 1.1 Completed GHRS/1 5417 (A Search for the Physical Processes on Jupiter) The High Resolution Spectrograph (Side One) was used as part of a program to observe atomic hydrogen emission at different latitudes and longitudes on the planet Jupiter ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_95/hst_status_09_08_95 -- 4.1 Кб -- 08.09.1995
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    7. http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_05_11_94
    ... 1.1 Completed Two Sets of GHRS/1 5417 (A Search for the Physical Processes on Jupiter) The High Resolution Spectrograph (Side One) was used as part of a program to observe atomic hydrogen emission at different latitude and longitudes on the planet Jupiter ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_05_11_94 -- 4.4 Кб -- 12.05.1994
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    8. http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_05_17_94
    ... 1.5 Completed GHRS/1 5417 (A Search for the Physical Processes on Jupiter) The High Resolution Spectrograph (Side One) was used as part of a program to observe atomic hydrogen emission at different latitude and longitudes on the planet Jupiter. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_94/hst_status_05_17_94 -- 7.1 Кб -- 18.05.1994
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    9. Publications for Ronald J. Allen
    ... Distribution and kinematics of the atomic and ionized hydrogen " Tilanus, R. P. J ... Atomic hydrogen produced in M33 photodissociation regions " Heiner, J. S.; Allen, R ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~rjallen/MyRefPubs.html -- 32.5 Кб -- 10.11.2011
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    10. The Birth of Stars: Herbig-Haro Jets, Accretion and Proto-Planetary Disks
    ... The total mass of molecular gas in the Galaxy is about 2 to 4 M and there is a comparable amount of atomic hydrogen (HI). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/ballyj.html -- 49.2 Кб -- 19.04.2006
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