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GOM08 - Radio Interferometric Observations of Candidate Water-Maser-Emitting Planetary Nebulae

Short title: Gomez et al. (2008)
Authors: Gómez, José F. Suárez, Olga Gómez, Yolanda Miranda, Luis F. Torrelles, José M. Anglada, Guillem Morata, Óscar
Journal: The Astronomical Journal, Volume 135, Issue 6, pp. 2074-2083 (2008).
Bibcode: 2008AJ....135.2074G

Detection table from Gomez et al. (2008)

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ID Obs. RA Obs. Dec l b Group id Source name Line Vrange Vpeak Fpeak Detection Class Dist. (parallax)
(J2000) (J2000) (deg.) (deg.) H2O (km/s) (km/s) (Jy) Yes/No (kpc)
117 47 35.3-29 50 57359.4423-0.8405G359.442-0.840
IRAS 17443-294922 GHz; -6.3;0.96.9-6.3+H2O +OH SFR_MIXED
218 01 19.6-31 11 22359.7780-4.0710G359.778-4.071
IRAS 17580-311122 GHz; 0.417.4+H2O +OH EVOLVED
318 09 12.4-25 04 345.9737-2.6110G5.974-2.611
IRAS 18061-250522 GHz; 57.4;63.95.760.7+H2O -OH EVOLVED
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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 GOM08

    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 GOM08 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

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    2MASS K

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