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ZIJ91 - IRAS 07027 - 7934 - The link between OH/IR stars and carbon-rich planetary nebulae

Short title: Zijlstra et al. (1991)
Authors: Zijlstra, A. A. Gaylard, M. J. te Lintel Hekkert, P. Menzies, J. Nyman, L.-A. Schwarz, H. E.
Journal: Astronomy and Astrophysics (ISSN 0004-6361), vol. 243, no. 1, March 1991, p. L9-L12.
Bibcode: 1991A&A...243L...9Z

Detection table from Zijlstra et al. (1991)

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ID Obs. RA Obs. Dec l b Group id Source name Frequency Vrange Vpeak Fpeak List Detection Ref.
(J2000) (J2000) (deg.) (deg.) (MHz) (km/s) (km/s) (Jy) Yes/No
106 59 26.4-79 38 47291.3750-26.2939G291.375-26.293
IRAS 07027-7934166751.0-51.00.600ENG15+OH ZIJ91
06 59 26.4-79 38 47291.3750-26.2939G291.375-26.293
IRAS 07027-793416127.0-47.05.200ENG15+OH ZIJ91
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Non-detection table from Zijlstra et al. (1991)

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ID Obs. RA Obs. Dec l b Group id Source name Fpeak List Detection Ref.
(J2000) (J2000) (deg.) (deg.) (Jy) Yes/No
106 59 26.4-79 38 47291.3750-26.2939G291.375-26.293
IRAS 07027-79340.500ENG15+OH ZIJ91
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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 ZIJ91

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

  • Distribution of sources from ZIJ91 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