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Data: CH3OH_I

BER92 - Observations of the methanol 4-1-30 E line in molecular clouds

Short title: Berulis et al. (1992)
Authors: Berulis, I. I. Kalenski, S. V. Sobolev, A. M. Streinitski, V. S.
Journal: Astronomical and Astrophysical Transactions, vol. 1, p. 231-245
Bibcode: 1992A&AT....1..231B

PDF: BER92.pdf

Detection table from Berulis et al. (1992)

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ID Obs. RA Obs. Dec l b Other name Line Vpeak FWHM Fpeak List Beam Ref.
(J2000) (J2000) (deg.) (deg.) Comp CH3OH (class I) (km/s) (km/s) (Jy) (arcsec)
117 47 16.8-28 21 17.50.6858-0.009136 GHz (I)
0.421052632AVE022BER92
217 49 20.6-27 34 8.51.59420.006336 GHz (I)
54.21.27E+02AVE022BER92
320 39 0.9+42 22 37.881.71910.569536 GHz (I)
0.20.81.22E+01AVE022BER92
417 45 37.9-29 05 45.7359.8648-0.085436 GHz (I)
5.74.01.75E+01AVE022BER92
519 23 42.6+14 31 3.349.4944-0.379236 GHz (I)
53.058.40E+00AVE022BER92
619 23 42.6+14 31 3.349.4944-0.379236 GHz (I)
55.37.07.80E+01AVE022BER92
717 47 20.8-28 23 17.20.6651-0.039036 GHz (I)
70.074.00E+02AVE022BER92
806 41 9.8+09 29 34.9203.31572.055236 GHz (I)
8.00.81.95E+04AVE022BER92
920 38 55+42 19 23.581.66510.5512West36 GHz (I)
-2.730.423.12E+01AVE022BER92
1020 39 0.9+42 21 57.981.71030.562736 GHz (I)
-2.83.51.52E+01AVE022BER92
1102 27 3.4+61 52 24.6133.94651.063936 GHz (I)
-46.24.4AVE022BER92
1202 27 3.4+61 52 24.6133.94651.063936 GHz (I)
-486.04.80E+00AVE022BER92
1320 39 0.9+42 21 57.981.71030.562736 GHz (I)
-551.55E+01AVE022BER92
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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 BER92

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

  • Distribution of sources from BER92 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