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Select data type: H2O, OH, CH3OH_II

SUN18 - Discovery of H2O, CH3OH, and OH Masers in the Extreme Outer Galaxy

Short title: Sun et al. (2018)
Authors: Sun, YanXu, YeChen, XiFang, MinHenkel, ChristianYang, JiMenten, Karl M.Chen, Xue-PengJiang, Zhi-Bo
Journal: The Astrophysical Journal, Volume 869, Issue 2, article id. 148, 13 pp. (2018).
Bibcode: 2018ApJ...869..148S

Detection table from Sun et al. (2018)

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ID Obs. RA Obs. Dec l b Group id Source name Frequency Vrange Vpeak FWHM Fpeak ∫F dv Telescope RMS Beam Detection Date
(J2000) (J2000) (deg.) (deg.) (MHz) (km/s) (km/s) (km/s) (Jy) (Jy*km/s) (Jy) (arcsec) Yes/No
118 58 18.3+01 15 57.734.8416-0.9500G34.842-0.950
34.84-0.954765-44.7;-44.1-44.40.090.370.09TMRT0.046180+H2O +OH 2017 June-August
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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 SUN18

    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 SUN18 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