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LIN92 - Discovery of bipolar OH maser emission from the high-latitude supergiant star HD 101584

Short title: te Lintel Hekkert et al. (1992)
Authors: te Lintel Hekkert, P. T. L. Chapman, J. M. Zijlstra, A. A.
Journal: Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 390, no. 1, May 1, 1992, p. L23-L26.
Bibcode: 1992ApJ...390L..23T

Detection table from te Lintel Hekkert et al. (1992)

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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
111 40 58.7-55 34 23.6293.02725.9377G293.028+5.937
IRAS 11385-5517166747.716.50.220ENG15+OH LIN92
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Non-detection table from te Lintel Hekkert et al. (1992)

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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
111 40 58.7-55 34 23.6293.02725.9377G293.028+5.937
IRAS 11385-55170.040ENG15+OH LIN92
11 40 58.7-55 34 23.6293.02725.9377G293.028+5.937
IRAS 11385-55170.060ENG15+OH LIN92
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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 LIN92

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

  • Distribution of sources from LIN92 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