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LIN88 - Two IRAS sources with high velocity outflow similar to OH231.8 + 4.2

Short title: te Lintel Hekkert et al. (1988)
Authors: te Lintel Hekkert, P. Habing, H. J. Caswell, J. L. Norris, R. P. Haynes, R. F.
Journal: Astronomy and Astrophysics (ISSN 0004-6361), vol. 202, no. 1-2, Aug. 1988, p. L19-L22.
Bibcode: 1988A&A...202L..19T

Detection table from te Lintel Hekkert et al. (1988)

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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
115 44 11.1-49 55 20329.14243.9498G329.142+3.950
IRAS 15405-4945161246.036.00.200ENG15-CH3OH II +OH LIN88
15 44 11.1-49 55 20329.14243.9498G329.142+3.950
IRAS 15405-4945166528.036.00.500ENG15-CH3OH II +OH LIN88
15 44 11.1-49 55 20329.14243.9498G329.142+3.950
IRAS 15405-4945166787.0-17.00.300ENG15-CH3OH II +OH LIN88
216 37 40-38 20 17344.07375.8466G344.074+5.847
IRAS 16342-38141612119.0-11.01.000ENG15+H2O +OH -SiO LIN88
16 37 40-38 20 17344.07375.8466G344.074+5.847
IRAS 16342-3814166562.019.00.500ENG15+H2O +OH -SiO LIN88
16 37 40-38 20 17344.07375.8466G344.074+5.847
IRAS 16342-3814166719.0-12.00.300ENG15+H2O +OH -SiO LIN88
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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 LIN88

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

  • Distribution of sources from LIN88 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