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Data: CH3OH_I

ELL17 - Class I methanol masers in NGC 253: Alcohol at the end of the bar

  Interferometry data

Short title: Ellingsen et al. (2017)
Authors: Ellingsen, S. P. Chen, X. Breen, S. L. Qiao, H.-H.
Journal: Monthly Notices of the Royal Astronomical Society, Volume 472, Issue 1, p.604-615
Bibcode: 2017MNRAS.472..604E

PDF: ELL17.pdf

Detection table from Ellingsen et al. (2017)

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ID Obs. RA Obs. Dec RA offset Dec offset l b Group id # Location Source name Image Line Vpeak Fpeak ∫F dv Telescope RMS Detection Date
(J2000) (J2000) (arcsec) (arcsec) (deg.) (deg.) CH3OH (class I) (km/s) (Jy) (Jy*km/s) (mJy/beam) Yes/No
1+00 47 31.93-25 17 29.197.216821-87.964982G97.224-87.965
NGC 253 Image 36 GHz (I)
143 .. 345.5 .. .. ATCA1.100+CH3OH I 2014 October 10, 11 and November 27, 28
+00 47 31.93-25 17 29.10 mas0 mas97.216821-87.9649821MM1NGC 253314
+00 47 31.96-25 17 29.10.44880 mas97.219699-87.9650302MM2NGC 253345.5
+00 47 32.04-25 17 25.81.64883.301297.238391-87.9643303MM3NGC 253275
+00 47 33.65-25 17 13.225.798815.901297.434808-87.9637424MM4NGC 253188
+00 47 33.67-25 17 11.926.098817.201297.441034-87.9634465MM5NGC 253143
+00 47 33.94-25 17 10.930.148818.201297.470276-87.9636256MM6NGC 253207.5
+00 47 34.13-25 17 1232.998817.101297.484894-87.9642057MM7NGC 253228.5
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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 ELL17

    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 ELL17 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