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    21. http://www.stsci.edu/jwst/news/2005/science-requirements.pdf
    ... JWST must be able to measure the [NeVI] line in an ultra-luminous obscured galaxy with the bolometric luminosity of Arp 220, 1.3в1012 L , at z ~ 2, assuming a line/bolometric luminosity ratio as in the Circinus galaxy, at 10 in less than 105 s (see Figure ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/news/2005/science-requirements.pdf -- 1600.7 Кб -- 05.02.2013
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    22. http://www.stsci.edu/ftp/instrument_news/FOC/Foc_isr/foc_isr083.ps
    ... and IUE m 220 magnitudes, while fig. 2 compares the ratio of F 220 fluxes F IUE =F FOC as a function of integrated count rate ... The FOC and IUE fluxes agree very well except for NGC 3690, which forms with IC 694 the merging system Arp 299. ...
    [ Текст ]  Ссылки http://www.stsci.edu/ftp/instrument_news/FOC/Foc_isr/foc_isr083.ps -- 169.2 Кб -- 28.02.1995
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    23. http://www.stsci.edu/hst/proposing/exp_abstract-catalogs/cy10-abstract-catalog
    ... Do these distant ultraluminous galaxies resemble local analogs (e.g., Arp 220)? ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/proposing/exp_abstract-catalogs/cy10-abstract-catalog -- 289.7 Кб -- 09.04.2003
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    24. http://www.stsci.edu/jwst/doc-archive/white-papers/SRD.pdf
    ... JWST will be able to measure the [NeVI] line in an ultra-luminous obscured galaxy with the bolometric luminosity of Arp 220, 1.3в1012 L ,at z 2, assuming a line/bolometric luminosity ratio as in the Circinus galaxy (Figure 9). ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/white-papers/SRD.pdf -- 2341.6 Кб -- 01.03.2014
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    25. http://www.stsci.edu/ftp/ExInEd/electronic_reports_folder/FOSI.pdf
    ... 8. Core of peculiar galaxy Arp 220. Credit: E. Shaya, D. Dowling (University of Maryland), WFPC IDT, NASA. 9. ...
    [ Текст ]  Ссылки http://www.stsci.edu/ftp/ExInEd/electronic_reports_folder/FOSI.pdf -- 1419.7 Кб -- 23.08.1995
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    26. http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-REF-000618.pdf
    ... However, even objects heavily obscured by dust, such as the Circinus Galaxy and bright star-forming galaxies, such as Arp 220, are quite luminous in the NIR and could easily be detected by NGST to comparable redshifts and with better angular resolution. ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-REF-000618.pdf -- 1674.9 Кб -- 05.02.2013
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    27. http://www.stsci.edu/institute/stuc/may-2014/solar-system.pdf
    ... T- Pyx nova TW Hydrae planetary gap Heritage Arp 142 comet ISON movie blue exoplanet Neptune moon Heritage: comet ISON GRB Kilonova Magellanic stream origin Galaxies in Fme M87 black hole jet movie Heritage "caterpillar" nebula ESA - planetary neb. ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/stuc/may-2014/solar-system.pdf -- 1222.5 Кб
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    28. Howard Bushouse's Publications
    ... ApJ 335 74 . "The Far-Infrared Structure of the Luminous Interacting Galaxy Arp 299." ... Imaging Survey of Interacting Galaxies: The Small Angular-Size Arp Systems ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~bushouse/pubs.html -- 32.8 Кб -- 15.03.2013
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    29. http://www.stsci.edu/~inr/post/maj1.ps
    ... 1996) and globular clusters associated with Sgr (Terzan 7, Terzan 8, Arp 2 and M54 ... velocity for the local standard of rest of 220 km s \Gamma1 and a solar motion with ...
    [ Текст ]  Ссылки http://www.stsci.edu/~inr/post/maj1.ps -- 1436.0 Кб -- 08.06.2007
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    30. http://www.stsci.edu/~bushouse/pubs/co_ii.ps.gz
    ... A complete SIG sample in the northern sky The complete sample of SIGs was compiled from the UGC (Nilson 1973), ARP catalog (Arp 1966) and the Catalogue of Isolated Pairs of Galaxies in the Northern Sky (CPG) (Karachentsev 1972). ...
    [ Текст ]  Ссылки http://www.stsci.edu/~bushouse/pubs/co_ii.ps.gz -- 138.0 Кб -- 06.09.2001
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