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Data: CH3OH_I

LIT11 - Search for class I methanol maser emission toward several supernova remnants

Short title: Litovchenko et al. (2011)
Authors: Litovchenko, I. D. Alakoz, A. V. Val'Tts, I. E. Larionov, G. M.
Journal: Astronomy Reports, Volume 55, Issue 11, pp.978-988
Bibcode: 2011ARep...55..978L

PDF: LIT11.pdf

Detection table from Litovchenko et al. (2011)

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ID Obs. RA Obs. Dec l b Source name Other name Line Vpeak FWHM Fpeak ∫F dv Telescope Beam Date
(J2000) (J2000) (deg.) (deg.) IRAS identification CH3OH (class I) (km/s) (km/s) (Jy) (Jy*km/s) (arcsec)
118 41 51-05 01 28.327.3686-0.163727.369-0.16418367-050444 GHz (I)
88.745(0.000)0.685(0.137)11.9528.712(1.062)ONSALA88December 2-15, 2009
218 41 51-05 01 28.327.3686-0.163727.369-0.16418367-050444 GHz (I)
91.108(0.000)0.950(0.000)15.57015.750(0.774)ONSALA88December 2-15, 2009
318 41 51-05 01 28.327.3686-0.163727.369-0.16418367-050444 GHz (I)
93.560(0.116)2.038(0.167)32.56270.632(8.208)ONSALA88December 2-15, 2009
418 41 51-05 01 28.327.3686-0.163727.369-0.16418367-050444 GHz (I)
94.466(0.005)0.767(0.034)84.36668.886(6.624)ONSALA88December 2-15, 2009
518 41 51-05 01 28.327.3686-0.163727.369-0.16418367-050444 GHz (I)
95.785(0.008)0.537(0.022)48.74427.882(1.350)ONSALA88December 2-15, 2009
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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

    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 LIT11

    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 LIT11 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