Display data from paper

Data: CH3OH_I

KAL94B - Observations of methanol masers at 95 GHz

Short title: Kalenskii et al. (1994B)
Authors: Kalenskii, S. V. Liljestroem, T. Val'tts, I. E. Vasil'kov, V. I. Slysh, V. I. Urpo, S.
Journal: Astronomy and Astrophysics Suppl., Vol. 103, p.129-134 (1994)
Bibcode: 1994A&AS..103..129K

PDF: KAL94B.pdf

Detection table from Kalenskii et al. (1994B)

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ID Obs. RA Obs. Dec l b Other name Line Vpeak FWHM ∫F dv List Beam Ref.
(J2000) (J2000) (deg.) (deg.) Comp CH3OH (class I) (km/s) (km/s) (Jy*km/s) (arcsec)
106 12 56.4+17 59 53.8192.5974-0.035595 GHz (I)
10.752.1297.00AVE0260KAL94B
219 23 43.9+14 30 36.449.4901-0.387195 GHz (I)
55.675.58300.00AVE0260KAL94B
306 41 9.7+09 29 34.9203.31552.054995 GHz (I)
7.240.83130.00AVE0260KAL94B
420 38 36.8+42 37 59.581.87750.7838(N)95 GHz (I)
9.051.9890.00AVE0260KAL94B
505 39 12.9+35 45 54173.48082.446195 GHz (I)
-171.57110.00AVE0260KAL94B
620 38 54.6+42 19 23.581.66440.552195 GHz (I)
-2.541.06290.00AVE0260KAL94B
720 39 3.5+42 25 5381.76700.5961S(3)95 GHz (I)
-4.472.3890.00AVE0260KAL94B
823 13 46.4+61 27 32.7111.54030.766495 GHz (I)
-57.551.31220.00AVE0260KAL94B
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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 KAL94B

    Tip: Use "Box select" or "Lasso select" to display velocity-selected sources in Aladin all-sky view

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

  • Distribution of sources from KAL94B 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