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Data: H2O

DEG10B - SiO Maser Survey off the Galactic Plane: A Signature of Streaming Motion

Short title: Deguchi et al. (2010B)
Authors: Deguchi, Shuji Shimoikura, Tomomi Koike, Kazutaka
Journal: Publications of the Astronomical Society of Japan, Vol.62, No.3, pp.525--546
Bibcode: 2010PASJ...62..525D

PDF: DEG10B.pdf

Detection table from Deguchi et al. (2010B)

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ID Obs. RA Obs. Dec l b Group id Source name Vpeak Fpeak ∫F dv Date RMS Detection
(J2000) (J2000) (deg.) (deg.) (km/s) (Jy) (Jy*km/s) (Jy) Yes/No
112 58 38.9+23 08 21.5325.571385.6903G325.570+85.690
J12583891+2308215 26.55.90168.4662009-05-300.351+SiO
215 28 43.7+03 49 438.103545.8400G8.104+45.840
J15284369+0349430 44.75.04932.7532009-05-300.306+H2O +OH +SiO
318 08 9.1-06 49 0521.87026.4181G21.870+6.418
J18080907-0649050 -56.51.03529.6612009-04-170.189+H2O +SiO
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  • Distribution of sources in all sky (l,b)

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  • Distribution of sources in all sky using Aladin

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  • Distribution of sources in IRAS color-color diagram

    Tip: Use "Box select" or "Lasso select" to display colour-selected sources in Aladin all-sky view

    Tip: Click on some source to look at the different surveys. You must select some surveys in previous page at "View images"

    Original color diagram is taken form van der Veen & Habing (1987)

    Type Description
    I Oxygen-rich non-variable stars without circumstellar shells
    II Variable stars with "young" O-rich circumstellar shells
    IIIa Variable stars with more evolved O-rich circumstellar shells
    IIIb Variable stars with thick O-rich circumstellar shells
    IV Variable stars with very thick O-rich circumstellar shells
    V Planetary nebulae and non- variable stars with very cool circumstellar shells
    VIa Variable stars with relatively cold dust at large distances; a significant part of the stars is carbon-rich
    VIb Variable stars with relatively hot dust close to the star and relatively cold dust at large distances; Some of the objects have proven to be O-rich
    VII Variable stars with more evolved C-rich circumstellar shells
    VIII Different sort of objects

  • Distribution of the detection velocities versus galactic longitude from DEG10B

    Tip: Use "Box select" or "Lasso select" to display velocity-selected sources in Aladin all-sky view

    Tip: Click on some source to look at the different surveys. You must select some surveys in previous page at "View images"

    Longitude-Velocity Map is taken form Dame, Hartmann & Thaddeus (2001)

  • Distribution of sources from DEG10B in (l,b) histograms



    X
    DSS colored
    2MASS colored
    WISE colored
    SDSS color
    IRAC color I1,I2,I4
    GLIMPSE 360
    PACS color (70-160 um)
    SPIRE color (250-500 um)
    NVSS (1.4GHz)
    ATLASGAL 870 um
    ATLASGAL 870 um + Planck
    Bolocam 1.1 mm
    UKIDSS K
    2MASS K