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Select data type: CH3OH_I

TUR72 - Detection of the 4_{1}-3_{0} (E_{2}) Line of Interstellar Methyl Alcohol

Short title: Turner et al. (1972)
Authors: Turner, B. E. Gordon, M. A. Wrixon, G. T.
Journal: Astrophysical Journal, vol. 177, p.609
Bibcode: 1972ApJ...177..609T

Detection table from Turner et al. (1972)

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ID Obs. RA Obs. Dec l b Group id Other name Line Vpeak FWHM Fpeak List Beam Detection Ref.
(J2000) (J2000) (deg.) (deg.) Comp CH3OH (class I) (km/s) (km/s) (Jy) (arcsec) Yes/No
117 47 21.5-28 24 8.20.6544-0.0486G0.667-0.036
36 GHz (I)
53.977.20E+01AVE021+H2O +CH3OH I +CH3OH II +OH +SiO TUR72
217 47 19.8-28 22 22.30.6762-0.0279G0.667-0.036
K136 GHz (I)
70.37AVE021+H2O +CH3OH I +CH3OH II +OH +SiO TUR72
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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

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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 TUR72

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

  • Distribution of sources from TUR72 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