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WIE04 - The polarization of mm methanol masers

Short title: Wiesemeyer et al. (2004)
Authors: Wiesemeyer, H. Thum, C. Walmsley, C. M.
Journal: Astronomy and Astrophysics, v.428, p.479-495 (2004)
Bibcode: 2004A&A...428..479W

Detection table from Wiesemeyer et al. (2004)

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ID Obs. RA Obs. Dec l b Group id Source name Image Line Vpeak FWHM Fpeak Telescope Detection Class Dist. (parallax) Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class II) (km/s) (km/s) (Jy) Yes/No (kpc)
123 13 45.4-61 28 9.7321.6255-51.9677G321.626-51.968
NGC 7538-IRS1 Image 107 GHz (II); -56.3<2.34<16.3IRAM+CH3OH II February and May 2002
23 13 45.4-61 28 9.7321.6255-51.9677G321.626-51.968
NGC 7538-IRS1107 GHz (II); -58.59<1.57<11.8IRAM+CH3OH II February and May 2002
23 13 45.4-61 28 9.7321.6255-51.9677G321.626-51.968
NGC 7538-IRS1107 GHz (II); -60.560.888.9IRAM+CH3OH II February and May 2002
422 56 18.1+62 01 49.5109.87122.1142G109.871+2.114
CepA157.0 GHz (II); -3.840.4819.5IRAM+H2O +CH3OH I +CH3OH II +OH SFRFebruary and May 2002
22 56 18.1+62 01 49.5109.87122.1142G109.871+2.114
CepA157.0 GHz (II); -2.80.3440.6IRAM+H2O +CH3OH I +CH3OH II +OH SFRFebruary and May 2002
22 56 18.1+62 01 49.5109.87122.1142G109.871+2.114
CepA157.0 GHz (II); -1.750.5717IRAM+H2O +CH3OH I +CH3OH II +OH SFRFebruary and May 2002
22 56 18.1+62 01 49.5109.87122.1142G109.871+2.114
CepA157.0 GHz (II); -1.30.5810.2IRAM+H2O +CH3OH I +CH3OH II +OH SFRFebruary and May 2002
818 06 14.8-20 31 329.62140.1953G9.621+0.195
G9.62+ 0.19157.0 GHz (II); 1.550.886.4IRAM+H2O +CH3OH I +CH3OH II +OH SFRFebruary and May 2002
18 06 14.8-20 31 329.62140.1953G9.621+0.195
G9.62+ 0.19157.0 GHz (II); -0.090.663.5IRAM+H2O +CH3OH I +CH3OH II +OH SFRFebruary and May 2002
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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

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    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 WIE04

    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 WIE04 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