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http://www.stecf.org/documents/isr/ISR_NGST_2002-02.pdf.

1. The Galaxy Gallery: Messier Objects
M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/messier.html -- 7.0 Кб -- 23.07.2004
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2. http://www.stsci.edu/jwst/doc-archive/st-ecf-documents/JWST-STScI-002267.pdf
JWST-STScI-002267 SOCCER Entry 10/5/2010 `On' failures in the NIRSpec MEMS ST-ECF Instrument Science Report NGST 2002-02 The effects of `on' failures in a MEMS array for the NGST NIRSpec Santiago Arribas, Robert Fosbury Peter Jakobsen --1-- JWST-STScI-002267 SOCCER Entry 10/5/2010 ST-ECF Instrument Science Report NGST 2002-02 The effects of `on' failures in a MEMS array for the NGST ... From this, we can decide on an acceptable number of facet failures. ...
[ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/st-ecf-documents/JWST-STScI-002267.pdf -- 1191.3 Кб -- 01.03.2014
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3. Gravitational Wave Background from Individual Galaxies
Next: Critical Frequencies and Gravitational Previous: Extragalactic Gravitational Wave Background . The number of binaries per frequency decade per solid angle from a separate stellar system (galaxy or cluster of galaxies) is . ... For example, for the Andromeda galaxy M31 ( rad, ) one gets . ... If the angular size of the galaxy is less than the angular resolution of the detector, the critical frequency is independent of the angular resolution, . ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node84.html -- 4.6 Кб -- 04.03.1997
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4. Arcsecond Positions of UGC Galaxies
... We measured these galaxies individually, and they are distinguished in our list by the suffixes a, b, c,... in order of increasing J2000 right ascension. ... The first column contains the UGC catalog number, to which we have added lower-case suffixes a, b, c,\dots in order of increasing J2000 right ascension to distinguish individual galaxies in groups. ... The third column lists the degrees, arcminutes, and arcseconds of J2000 declination plus the rms uncertainty in arcseconds. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/UGC.html -- 3.7 Кб -- 18.03.2015
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5. The Galaxy NGC 3882
... Figures 1 and 2: Neutral hydrogen distribution (top) and mean velocity field (bottom) of the galaxy NGC 3882 (v = 1817 km/s) and a new companion galaxy, ATCA J1147-56 (v = 1760 km/s). ... The total HI flux densities are about 32.4 Jy km/s for NGC3882 and 0.6 Jy km/s for ATCA J1147-56; beam size: 107 arcsec x 88 arcsec. ... Figure 6: ATCA HI global spectrum of the new galaxy, ATCA J1147-56. ... Figure 7: HIPASS spectrum of NGC 3882 (v = 1817 km/s). bkoribal @ atnf.csiro.au ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Baerbel.Koribalski/ngc3882/ -- 3.2 Кб -- 02.10.2012