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VOR05 - The 6.7- and 25-GHz methanol masers in OMC-1

  Interferometry data

Short title: Voronkov et al. (2005)
Authors: Voronkov, M. A. Sobolev, A. M. Ellingsen, S. P. Ostrovskii, A. B.
Journal: Monthly Notices of the Royal Astronomical Society, Volume 362, Issue 3, pp. 995-1005.
Bibcode: 2005MNRAS.362..995V

Detection table from Voronkov et al. (2005)

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ID Obs. RA Obs. Dec RA offset Dec offset l b Group id # Source name Image Line Vpeak Fpeak ∫F dv Major Minor PA Telescope Beam Detection Date
(J2000) (J2000) (arcsec) (arcsec) (deg.) (deg.) CH3OH (class II) (km/s) (Jy) (Jy*km/s) (arcsec) (arcsec) (deg.) (arcsec) Yes/No
1+05 35 15-05 23 42.53209.012979-19.391939G209.015-19.405
OMC-1 Image 6.6 GHz (II)
-1.1 .. 7.90.17 .. 0.45 .. ATCA432+H2O +CH3OH I +CH3OH II 2003 June - 2004 april
+05 35 13.93-05 24 5.3-16.05-22.7708209.016831-19.3987581OMC-1-1.10.45 (0.03)31.00010.000-1.000
+05 35 14.77-05 22 49-3.4553.5292208.998463-19.3860642OMC-17.20.20 (0.03)53.00014.000-7.000
+05 35 14.6-05 22 37-665.5292208.994973-19.3851853OMC-17.30.19 (0.02)44.00016.000-13.000
+05 35 14.53-05 22 42-7.0560.5292208.996147-19.3860724OMC-17.50.22 (0.02)43.00017.0000.000
+05 35 14.37-05 22 46-9.4556.5292208.996879-19.3871675OMC-17.90.17 (0.01)40.00017.000-5.000
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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 VOR05

    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 VOR05 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