1,725,096 research outputs found

    UMNH:Mamm:2903

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    UMNH:Mamm:2903 Voucher specimen study ski

    D-2903: Unidentified residence

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    D-2903: Unidentified residenc

    Santa Fe (ATSF) 2903

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    A photograph postcard showing the Santa Fe (ATSF) 2903, 4-8-4, with a mixed freight

    Santa Fe (ATSF) 2903

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    A photograph print showing Santa Fe 2903, 4-8-4, Topeka, KS

    Santa Fe (ATSF) 2903 & 1806

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    A photograph postcard showing Santa Fe (ATSF) 2903, 4-8-4, on extra 2903 West, mixed freight, starting up Curtis Hill, just west of Waynoka, OK., 85 cars, 45 mph, with engine 1806 (obscured by smoke), 2-6-2, helping at rear. 10:25am, Plains Division

    Astronomische Nachrichten, nos 2890-2903

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    R. R. Astronomische Nachrichten, nos 2890-2903. In: Bulletin astronomique, tome 6, 1889. pp. 330-336

    Santa Fe (ATSF) 2903 & 1806

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    A photograph postcard showing Santa Fe (ATSF) 2903, 4-8-4, on head end of 85 car mixed freight with locomotive 1806 helping on rear

    Santa Fe (ATSF) 2903 & 1805

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    A photograph postcard showing Santa Fe (ATSF) 1805, 2-6-2,helping at rear of westbound freight extra EXA 2903 west, as it climbs Curtis Hill between Heman and Belva, OK, 113 cars, 25 mph. Plains Division [see also 2008.008.0304

    Star-forming regions in NGC 2903 bar (Popping+, 2010)

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    To investigate the extinction and the star-formation in the bar of NGC 2903 we used the Spitzer 24um observations from the Multiband Imaging Photometer (MIPS) instrument. To analyse the UV emission and its distribution in NGC 2903, we used GALEX mission data. Ground-based optical images from the Sloan Digital Sky Survey (SDSS) and a map of the CO (J=1-0) rotational transition emission were also used for the morphological analysis of NGC 2903. (2 data files)

    Star-forming regions in NGC 2903 bar (Popping+, 2010)

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    To investigate the extinction and the star-formation in the bar of NGC 2903 we used the Spitzer 24um observations from the Multiband Imaging Photometer (MIPS) instrument. To analyse the UV emission and its distribution in NGC 2903, we used GALEX mission data. Ground-based optical images from the Sloan Digital Sky Survey (SDSS) and a map of the CO (J=1-0) rotational transition emission were also used for the morphological analysis of NGC 2903. (2 data files)
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