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Select data type: CH3OH_II

MOS17 - Extended CH3OH maser flare excited by a bursting massive YSO

Short title: Moscadelli et al. (2017)
Authors: Moscadelli, L.Sanna, A.Goddi, C.Walmsley, M. C.Cesaroni, R.Caratti o Garatti, A.Stecklum, B.Menten, K. M.Kraus, A.
Journal: Astronomy & Astrophysics, Volume 600, id.L8, 5 pp.
Bibcode: 2017A&A...600L...8M

Detection table from Moscadelli et al. (2017)

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ID Obs. RA Obs. Dec l b Group id Source name Image Line Vpeak Fpeak Telescope Beam Detection Class Dist. (parallax) Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class II) (km/s) (Jy) (arcsec) Yes/No (kpc)
106 12 54+17 59 23.5192.6002-0.0480G192.599-0.048
S255 NIRS 3 Image 6.6 GHz (II); 6.431006EVN0.005+H2O +CH3OH I +CH3OH II SFR_MIXED2016 April 12
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  • Distribution of sources in all sky (l,b)

    0

  • Distribution of sources in all sky using Aladin

    Tip: Click on some source to get more informaiton


  • 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

    Tip: Click on some source to look at the different surveys. You must select some surveys in previous page at "View images"

    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 MOS17

    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 MOS17 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

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    2MASS K

    Download 2MASS K FITS