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Data: CH3OH_I

MCC17 - Detection of 36 GHz Class I Methanol Maser Emission toward NGC 4945

Short title: McCarthy et al. (2017)
Authors: McCarthy, Tiege P. Ellingsen, Simon P. Chen, Xi Breen, Shari L. Voronkov, Maxim A. Qiao, Hai-hua
Journal: The Astrophysical Journal, Volume 846, Issue 2, article id. 156, 5 pp. (2017).
Bibcode: 2017ApJ...846..156M

PDF: MCC17.pdf

Detection table from McCarthy et al. (2017)

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ID Obs. RA Obs. Dec l b Source name Line Vpeak Fpeak Telescope Beam Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (km/s) (mJy) (arcsec)
113 05 28.1-49 28 12.3305.273713.3379NGC 494536 GHz (I)
67443.8ATCA262015 August 25 and 26
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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 MCC17

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

  • Distribution of sources from MCC17 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