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    11. GHRS Observations of Interstellar Deuterium toward HZ 43
    ... hydrogen NLTE atmosphere, (2) a deuterium abundance and thermal broadening parameter consistent with those derived toward ... a pure hydrogen model atmosphere with T = 49,000 K, and = 7.7, as derived by Napiwotzki et al. (1993), (2) a hydrogen column ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/landsmanw.html -- 15.9 Кб -- 15.06.2005
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    12. 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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    13. Stars as Observed in the Infrared
    ... than about 3000 K effective temperature radiate like a hot blackbody at these long wavelengths, possibly with a very few atomic lines (of Hydrogen, in the A-type stars) or molecular bands (the CO band overtone near 2.25 microns for example, in K-type ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~volk/stars.html -- 4.1 Кб -- 14.06.2010
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    14. Starburst and Galaxy Evolution
    ... Far-ultraviolet observations of molecular hydrogen in the diffuse interstellar medium of starburst galaxies . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/starburst99/CCGI/Preprints2004.cgi -- 5.5 Кб -- 10.04.2016
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    15. The Spitzer Infrared Nearby Galaxies Survey: A High-Resolution Spectroscopy
    ... The fluxes for nine atomic forbidden and three molecular hydrogen mid-infrared emission lines are also provided, along with upper limits in key lines for infrared-faint targets. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2009ApJ...693.1821D.html -- 5.0 Кб -- 21.01.2016
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    16. Star Formation Rates in Resolved Galaxies: Calibrations with Near- and
    ... We use the near-infrared BrнЕ hydrogen recombination line as a reference star formation rate (SFR) indicator to test the validity and establish the calibration of the Herschel/PACS 70 нјm emission as a SFR tracer for sub-galactic regions in external ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2013ApJ...768..180L.html -- 5.4 Кб -- 21.01.2016
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    17. FUSE Measurements of Far-Ultraviolet Extinction. III. The Dependence on R(V)
    ... Molecular hydrogen absorption features were removed using individualized H2 models for each sightline. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2009ApJ...705.1320G.html -- 4.6 Кб -- 21.01.2016
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    18. Star Formation in NGC 5194 (M51a): The Panchromatic View from GALEX to Spitzer
    ... accurate local SFR tracer for the H II knots in NGC 5194, with a peak-to-peak dispersion of less than a factor of 3 relative to hydrogen emission line tracers; this suggests that the 24 ЮМm emission carriers are mainly heated by the young, ionizing stars ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2005ApJ...633..871C.html -- 6.4 Кб -- 21.01.2016
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    19. 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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    20. http://www.stsci.edu/ftp/instrument_news/FOS/pub/fos_scs_isr002_a.txt
    ... to 10000A, the FOS flux spectrum for G191B2B (WD0501+527) is divided by a model spectrum for the case of a pure hydrogen atmosphere to derive the difference between the current HST flux scale and the flux scale defined by the physics of model atmosphere ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/instrument_news/FOS/pub/fos_scs_isr002_a.txt -- 1.7 Кб -- 11.10.1995
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