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Data: CH3OH_I

BEU05 - High Spatial Resolution Observations of NH3 and CH3OH toward the Massive Twin Cores NGC 6334I and NGC 6334I(N)

  Interferometry data

Short title: Beuther et al. (2005)
Authors: Beuther, H. Thorwirth, S. Zhang, Q. Hunter, T. R. Megeath, S. T. Walsh, A. J. Menten, K. M.
Journal: The Astrophysical Journal, Volume 627, Issue 2, pp. 834-844.
Bibcode: 2005ApJ...627..834B      BiBTeX

PDF: BEU05.pdf

Detection table from Beuther et al. (2005)

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ID Obs. RA Obs. Dec RA offset Dec offset l b # Source name Image Descr. Line Vpeak Fpeak ∫F dv Telescope RMS Beam
(J2000) (J2000) (arcsec) (arcsec) (deg.) (deg.) CH3OH (class I) (km/s) (Jy) (Jy*km/s) (mJy) (arcsec)
1+17 20 53.44-35 47 2.2351.4167840.644896NGC 6334I Image Descr 24.928 GHz (I)
-5 .. -3 .. .. ATCA6.000130
+17 20 55.68-35 45 0.233.5988121.998351.4489440.6579981NGC 6334I-3
+17 20 55.03-35 45 1523.8488107.198351.4443130.6574602NGC 6334I-5
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Non-detection table from Beuther et al. (2005)

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ID Obs. RA Obs. Dec l b Source name Descr. Line Telescope RMS Beam
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (mJy) (arcsec)
1+17 20 54.63-35 45 8.9351.4449340.659537NGC 6334I (N) Descr 24.928 GHz (I)
ATCA6.000130
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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 BEU05

    Tip: Use "Box select" or "Lasso select" to display velocity-selected sources in Aladin all-sky view

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

  • Distribution of sources from BEU05 in (l,b) histograms



    X
    Position of H2O maser detection
    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