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BAT88 - Detection of a strong new maser line of methanol toward DR 21(OH)

  Interferometry data

Short title: Batrla & Menten (1988)
Authors: Batrla, Wolfgang Menten, Karl M.
Journal: Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 329, June 15, 1988, p. L117-L120. Research supported by the University of Illinois.
Bibcode: 1988ApJ...329L.117B

Detection table from Batrla & Menten (1988)

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ID Obs. RA Obs. Dec RA offset Dec offset l b Group id # Location Source name Line Vpeak Ta ∫Ta dv Beam PA Detection
(J2000) (J2000) (arcsec) (arcsec) (deg.) (deg.) CH3OH (class I) (km/s) (K) (K*km/s) (arcsec) (deg.) Yes/No
1+20 39 1.41467+42 22 37.880781.7200480.568267G81.699+0.563
DR 21(OH)84 GHz (I)
-1.56 .. 0.5314.9 .. 136.21 .. 8.3 x 6.256+H2O +CH3OH I +CH3OH II +OH -SiO
+20 38 59.8066+45 37 59.8804-24.121172284.3037922.55123511DR 21(OH)0.53(0.01)136.21(2.55)
+20 39 0.291893+42 22 46.7404-16.848.8681.7198990.57250722DR 21(OH)0.07(0.02)41.16(3.25)
+20 39 0.343893+42 22 46.5004-16.068.6281.7199440.57234032DR 21(OH)-0.51(0.11)20.90(3.68)
+20 39 0.39856+42 22 46.7604-15.248.8881.7201030.57225042DR 21(OH)-1.56(0.10)14.90(1.86)
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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 BAT88

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

  • Distribution of sources from BAT88 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