Contains:IC 1795, NGC 896

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    IC 1795, 




    

        Theodore Arampatz...
    IC 1795

    Technical card

    Resolution: 4230x2828

    Dates: Oct. 3, 2015

    Frames: 60x420"

    Integration: 7.0 hours

    Avg. Moon age: 20.76 days

    Avg. Moon phase: 64.52%

    Astrometry.net job: 802422

    RA center: 36.721 degrees

    DEC center: 62.061 degrees

    Pixel scale: 0.909 arcsec/pixel

    Orientation: -179.189 degrees

    Field radius: 0.643 degrees

    Locations: Παρατηρητήριο σπιτιού, Paramithia, Greece

    Description

    IC 1795 is an emission nebula located about 6,000 light-years away in the constellation Cassiopeia.
    The dominant central star of IC 1795 is a blue dwarf on the main sequence. In addition there are three other stars of class O and B with ages between 3 and 5 million years. This being an age intermediate to the 6 to 20 million years of the shell structure that encloses the complex. The region is one of the sites most studied (besides Orion) for the formation of massive stars. This area is more dense and rich in H II. It is home to, and hides, a group of young blue stars, with their radiation ionizing the residual gas clouds. (WIKI).

    Instruments and exposure data:
    W.O FLT110 with dedicated TMB field flattener
    FeatherTouch 3'' focuser
    Starizona MicroTouch autofocuser
    W.O ZS80 ED
    SBIG ST10XME CFW9
    Meade DSI
    Filters: Ha 5nm Astrodon
    Sky-Watcher EQ6 Pro

    Ha:60*7min bin1x1
    Total exposure time:7h

    Location: Vironas,Athens Greece

    Comments

    Author

    arasteo
    Theodore Arampatz...
    License: Attribution-NonCommercial-NoDerivs Creative Commons
    7999
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    IC 1795, 




    

        Theodore Arampatz...