Display data from paper

Data: CH3OH_I

SLY97 - Detection of a New Methanol Maser Line with the Kitt Peak 12 Meter Telescope by Remote Observing from Moscow

Short title: Slysh et al. (1997)
Authors: Slysh, V. I. Kalenskii, S. V. Val'tts, I. E. Golubev, V. V.
Journal: The Astrophysical Journal, Volume 478, Issue 1, pp. L37-L40.
Bibcode: 1997ApJ...478L..37S

PDF: SLY97.pdf

Detection table from Slysh et al. (1997)

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ID Obs. RA Obs. Dec l b Line Vpeak FWHM Fpeak List Beam Ref.
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (km/s) (km/s) (Jy) (arcsec)
120 39 0.7+42 22 50.881.72160.5722132.8 GHz (I)
0.280.866.34E+01AVE0240SLY97
218 04 53.9-24 26 41.36.0499-1.4493132.8 GHz (I)
10.612.681.29E+01AVE0240SLY97
318 04 53.9-24 26 41.36.0499-1.4493132.8 GHz (I)
10.920.775.52E+01AVE0240SLY97
418 29 24.8-15 15 48.916.8683-2.1582132.8 GHz (I)
16.3912.631.16E+01AVE0240SLY97
518 29 24.8-15 15 48.916.8683-2.1582132.8 GHz (I)
17.690.801.05E+01AVE0240SLY97
618 29 24.8-15 15 48.916.8683-2.1582132.8 GHz (I)
18.964.814.09E+01AVE0240SLY97
718 29 24.8-15 15 48.916.8683-2.1582132.8 GHz (I)
20.241.201.88E+01AVE0240SLY97
818 14 11.1-17 55 57.412.7968-0.1928132.8 GHz (I)
32.781.021.50E+01AVE0240SLY97
918 14 11.1-17 55 57.412.7968-0.1928132.8 GHz (I)
36.763.572.33E+01AVE0240SLY97
1006 41 9.7+09 29 34.9203.31552.0549132.8 GHz (I)
7.540.841.13E+01AVE0240SLY97
1106 41 9.7+09 29 34.9203.31552.0549132.8 GHz (I)
7.943.771.74E+01AVE0240SLY97
1220 39 0.7+42 22 50.881.72160.5722132.8 GHz (I)
-2.345.655.67E+01AVE0240SLY97
1320 38 54.6+42 19 23.581.66440.5521132.8 GHz (I)
-2.470.626.47E+01AVE0240SLY97
1420 38 54.6+42 19 23.581.66440.5521132.8 GHz (I)
-2.764.201.13E+01AVE0240SLY97
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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

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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 SLY97

    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 SLY97 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