Display data from paper

Data: CH3OH_I

ELL14 - Detection of 36 GHz Class I Methanol Maser Emission toward NGC 253

  Interferometry data

Short title: Ellingsen et al. (2014)
Authors: Ellingsen, Simon P. Chen, Xi Qiao, Hai-Hua Baan, Willem An, Tao Li, Juan Breen, Shari L.
Journal: The Astrophysical Journal Letters, Volume 790, Issue 2, article id. L28, 5 pp. (2014).
Bibcode: 2014ApJ...790L..28E

PDF: ELL14.pdf

Detection table from Ellingsen et al. (2014)

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ID Obs. RA Obs. Dec RA offset Dec offset l b # Source name Image Line Vpeak Fpeak ∫F dv Telescope Beam Date
(J2000) (J2000) (arcsec) (arcsec) (deg.) (deg.) CH3OH (class I) (km/s) (mJy) (mJy*km/s) (arcsec)
1+00 47 33.1-25 17 1897.366075-87.96407NGC 253 Image 36 GHz (I)
194 .. 3508.7 .. 10.5310ATCA8 x 4.22014 March 29
+00 47 33.8-25 17 1210.49885.998897.453188-87.9636791NGC 25319410.5310 (50)
+00 47 32-25 17 28-16.5012-10.001297.227210-87.9648182NGC 2533508.7310 (50)
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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 ELL14

    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 ELL14 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