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Data: CH3OH_I

VOR11 - Discovery of the new class I methanol maser transition at 23.4 GHz

Short title: Voronkov et al. (2011)
Authors: Voronkov, M. A. Walsh, A. J. Caswell, J. L. Ellingsen, S. P. Breen, S. L. Longmore, S. N. Purcell, C. R. Urquhart, J. S.
Journal: Monthly Notices of the Royal Astronomical Society, Volume 413, Issue 4, pp. 2339-2344.
Bibcode: 2011MNRAS.413.2339V      BiBTeX

PDF: VOR11.pdf

Detection table from Voronkov et al. (2011)

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ID Obs. RA Obs. Dec l b Source name Image Line Vpeak FWHM Fpeak ∫F dv Telescope Beam
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (km/s) (km/s) (Jy) (Jy*km/s) (arcsec)
117 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.16 Image 24.934 GHz (I)
-4.710.224 (4)1.43 (2)0.34 (3)ATCA120
217 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1624.928 GHz (I)
-5.530.25 (3)0.22 (2)1.8 (2)ATCA120
317 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1624.928 GHz (I)
-5.140.25 (2)0.39 (2)ATCA120
417 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1624.928 GHz (I)
-4.6650.333 (2)4.67 (2)ATCA120
517 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1624.933 GHz (I)
-5.640.30 (3)0.32 (2)2.1 (2)ATCA120
617 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1624.933 GHz (I)
-5.280.23 (1)0.70 (2)ATCA120
717 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1624.933 GHz (I)
-4.7660.399 (2)4.32 (2)ATCA120
817 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1624.959 GHz (I)
-5.630.33 (3)0.37 (2)2.2 (2)ATCA120
917 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1624.959 GHz (I)
-5.2650.24 (1)0.74 (2)ATCA120
1017 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1624.959 GHz (I)
-4.7440.392 (2)4.60 (2)ATCA120
1117 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1625.0 GHz (I)
-5.670.34 (4)0.31 (2)2.0 (2)ATCA120
1217 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1625.0 GHz (I)
-5.3020.27 (2)0.53 (2)ATCA120
1317 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1625.0 GHz (I)
-4.7880.433 (3)3.78 (2)ATCA120
1417 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1625.1 GHz (I)
-5.630.30 (2)0.56 (2)2.7 (3)ATCA120
1517 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1625.1 GHz (I)
-4.950.50 (1)3.87 (8)ATCA120
1617 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1625.1 GHz (I)
-4.640.33 (2)1.4 (2)ATCA120
1717 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1625.2 GHz (I)
-5.6250.28 (2)0.49 (3)2.6 (3)ATCA120
1817 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1625.2 GHz (I)
-4.960.48 (2)3.94 (8)ATCA120
1917 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1625.2 GHz (I)
-4.640.33 (2)1.5 (2)ATCA120
2017 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1623 GHz (I)
-5.5840.191 (8)1.00 (4)11 (1)ATCA120
2117 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1623 GHz (I)
-4.9320.450 (5)16.4 (2)ATCA120
2217 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.1623 GHz (I)
-4.6750.301 (4)8.6 (4)ATCA120
2317 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.169.93 GHz (I)
-5.4930.30 (1)6.1 (1)40 (1)ATCA120
2417 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.169.93 GHz (I)
-4.890.44 (2)50 (2)ATCA120
2517 41 19.1-30 44 58.1357.9670-0.1581G357.97-0.169.93 GHz (I)
-4.6380.34 (7)41 (4)ATCA120
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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

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

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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 VOR11

    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 VOR11 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