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Reference: [BD2002]

Detection table from BD2002

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ID Obs. RA Obs. Dec l b Group id Source name Other name Frequency Vpeak Fpeak List Detection Class Dist. (parallax) Ref.
(J2000) (J2000) (deg.) (deg.) (MHz) (km/s) (Jy) Yes/No (kpc)
102 27 3.9+61 52 24.6133.94741.0642G133.949+1.064
W3(OH)IRAS02232+613813441-43.045.300QIA14+H2O +CH3OH I +CH3OH II +OH SFRBD2002
02 27 3.9+61 52 24.6133.94741.0642G133.949+1.064
W3(OH)13435-45.2QIA14+H2O +CH3OH I +CH3OH II +OH SFRBD2002
320 10 9.1+31 31 34.469.5399-0.9760G69.540-0.976
IRAS20081+3122ON113441-0.30.950QIA14+H2O +CH3OH I +CH3OH II +OH SFRBD2002
421 43 1.4+54 56 16.398.03541.4458G98.035+1.446
IRAS21413+544213441-61.50.770QIA14+H2O +CH3OH I +CH3OH II +OH SFRBD2002
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  • Distribution of sources in all sky (l,b)

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  • Distribution of sources in all sky using Aladin

    Tip: Click on some source to get more informaiton


  • 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 BD2002

    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 BD2002 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

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    2MASS K

    Download 2MASS K FITS