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GRE04 - A Survey for Water Maser Emission toward Planetary Nebulae: New Detection in IRAS 17347-3139

Short title: de Gregorio-Monsalvo et al. (2004)
Authors: de Gregorio-Monsalvo, Itziar Gómez, Yolanda Anglada, Guillem Cesaroni, Riccardo Miranda, Luis F. Gómez, José F. Torrelles, José M.
Journal: The Astrophysical Journal, Volume 601, Issue 2, pp. 921-929.
Bibcode: 2004ApJ...601..921D

Detection table from de Gregorio-Monsalvo et al. (2004)

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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 38 0.7-31 40 54356.8016-0.0554G356.802-0.055
IRAS 17347-313922 GHz; -68.2;-61.8-68.10.7+H2O +OH SFR_MIXED
17 38 0.7-31 40 54356.8016-0.0554G356.802-0.055
IRAS 17347-313922 GHz; -68.2;-61.8-61.81.36+H2O +OH SFR_MIXED
17 38 0.7-31 40 54356.8016-0.0554G356.802-0.055
IRAS 17347-313922 GHz; -68.2;-61.8-68.21.7+H2O +OH SFR_MIXED
17 38 0.7-31 40 54356.8016-0.0554G356.802-0.055
IRAS 17347-313922 GHz; -68.2;-61.8-62.12.1+H2O +OH SFR_MIXED
519 27 44+21 30 3.456.09602.0937G56.096+2.094
K3-3522 GHz; 22.40.27+H2O +OH EVOLVED
19 27 44+21 30 3.456.09602.0937G56.096+2.094
K3-3522 GHz; 22.60.933+H2O +OH EVOLVED
19 27 44+21 30 3.456.09602.0937G56.096+2.094
K3-3522 GHz; 22.41.33+H2O +OH EVOLVED
19 27 44+21 30 3.456.09602.0937G56.096+2.094
K3-3522 GHz; 22.41.41+H2O +OH EVOLVED
19 27 44+21 30 3.456.09602.0937G56.096+2.094
K3-3522 GHz; 22.41.33+H2O +OH EVOLVED
19 27 44+21 30 3.456.09602.0937G56.096+2.094
K3-3522 GHz; 22.42.1+H2O +OH EVOLVED
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  • Distribution of sources in all sky (l,b)

    0

  • 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

    Tip: Click on some source to look at the different surveys. You must select some surveys in previous page at "View images"

    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 GRE04

    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 GRE04 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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