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SLY93 - The detection of a new methanol maser transition at 9.9 GHz

Short title: Slysh et al. (1993)
Authors: Slysh, V. I. Kalenskij, S. V. Val'tts, I. E.
Journal: Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 413, no. 2, p. L133-L135.
Bibcode: 1993ApJ...413L.133S

Detection table from Slysh et al. (1993)

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ID Obs. RA Obs. Dec l b Group id Source name Line Thermal Vpeak FWHM Fpeak Telescope Beam Detection
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) line mark (km/s) (km/s) (Jy) (arcsec) Yes/No
105 35 14.5-05 22 26.6208.9920-19.3843G208.993-19.385
Orion-KL9.93 GHz (I)
*8.7 (0.2)2.4 (0.3)0.25 (0.04)GBT204+H2O +CH3OH I +CH3OH II +OH +SiO
217 47 20.1-28 23 4.30.6668-0.0349G0.667-0.036
Sgr B29.93 GHz (I)
*62.5 (0.1)14.3 (0.2)0.19 (0.03)GBT204+H2O +CH3OH I +CH3OH II +OH +SiO
317 47 20.1-28 23 4.30.6668-0.0349G0.667-0.036
Sgr B210.05 GHz
*65150.04dGBT204+H2O +CH3OH I +CH3OH II +OH +SiO
418 14 10.7-17 55 53.412.7970-0.1908G12.797-0.193
W33-Met9.93 GHz (I)
33.5 (0.02)0.4 (0.01)0.80 (0.10)GBT204+H2O +CH3OH I +CH3OH II
518 14 10.7-17 55 53.412.7970-0.1908G12.797-0.193
W33-Met9.97 GHz
370.50.17GBT204+H2O +CH3OH I +CH3OH II
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Non-detection table from Slysh et al. (1993)

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ID Obs. RA Obs. Dec l b Group id Source name Line Fpeak Telescope Beam Detection
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (Jy) (arcsec) Yes/No
105 35 14.5-05 22 26.6208.9920-19.3843G208.993-19.385
Orion-KL9.97 GHz
<0.11bGBT204+H2O +CH3OH I +CH3OH II +OH +SiO
205 35 14.5-05 22 26.6208.9920-19.3843G208.993-19.385
Orion-KL10.05 GHz
<0.11GBT204+H2O +CH3OH I +CH3OH II +OH +SiO
317 47 20.1-28 23 4.30.6668-0.0349G0.667-0.036
Sgr B29.97 GHz
<0.019bGBT204+H2O +CH3OH I +CH3OH II +OH +SiO
418 14 10.7-17 55 53.412.7970-0.1908G12.797-0.193
W33-Met10.05 GHz
<0.13bGBT204+H2O +CH3OH I +CH3OH II
×
  • 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 SLY93

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

  • Distribution of sources from SLY93 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