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NAK86 - Molecular line observations of the S235B region

Short title: Nakano & Yoshida (1986)
Authors: Nakano, Makoto Yoshida, Shigeomi
Journal: Astronomical Society of Japan, Publications (ISSN 0004-6264), vol. 38, no. 4, 1986, p. 531-545. Research supported by the Japan Society for the Promotion of Science.
Bibcode: 1986PASJ...38..531N

Detection table from Nakano & Yoshida (1986)

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ID Obs. RA Obs. Dec l b Group id Other name Line Vpeak FWHM List Beam Detection Ref.
(J2000) (J2000) (deg.) (deg.) Comp CH3OH (class I) (km/s) (km/s) (arcsec) Yes/No
105 40 53.5+35 41 38.8173.72152.6971G173.719+2.698
max95 GHz (I)
-16.50.7AVE0220+H2O +CH3OH I +CH3OH II -OH NAK86
05 40 53.5+35 41 38.8173.72152.6971G173.719+2.698
max95 GHz (I)
-17.5AVE0220+H2O +CH3OH I +CH3OH II -OH NAK86
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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 NAK86

    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 NAK86 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