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ZEL90 - The discrete nature of circumstellar OH maser emission

Short title: Zell & Fix (1990)
Authors: Zell, Philip J. Fix, John D.
Journal: Astronomical Journal, vol. 99, Jan. 1990, p. 314-322.
Bibcode: 1990AJ.....99..314Z

Detection table from Zell & Fix (1990)

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ID Obs. RA Obs. Dec l b Group id Source name Frequency Vrange Vpeak Fpeak List Detection Class Dist. (parallax) Ref.
(J2000) (J2000) (deg.) (deg.) (MHz) (km/s) (km/s) (Jy) Yes/No (kpc)
119 14 19.5+11 10 3445.47070.0764G45.471+0.076
OH45.5+0.1161234.617.84.100ENG15-H2O +OH +SiO EVOLVEDZEL90
219 09 8.2+08 16 3442.3084-0.1324G42.308-0.132
OH42.3-0.1161233.042.36.000ENG15+H2O +OH +SiO EVOLVEDZEL90
318 58 30+06 42 5739.71281.4952G39.713+1.495
OH39.7+1.5161232.42.436.200ENG15+H2O +OH +SiO EVOLVEDZEL90
401 06 25.9+12 35 54128.6411-50.1071G128.642-50.107
WX PSC161236.8-9.919.700ENG15+H2O +OH +SiO EVOLVEDZEL90
519 06 22.2+08 13 4841.95230.4541G41.952+0.454
R AQL161212.642.61.500ENG15+H2O -CH3OH I +OH +SiO EVOLVEDZEL90
618 57 27.2+02 12 1735.5797-0.3322G35.580-0.333
OH35.6-0.3161229.062.021.000ENG15-H2O +OH +SiO SFR_MIXEDZEL90
719 31 25.2+18 13 1153.6302-0.2385G53.630-0.239
OH53.6-0.2161227.0-3.07.200ENG15-H2O +OH EVOLVEDZEL90
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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 ZEL90

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

  • Distribution of sources from ZEL90 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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