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LEW00 - On the Transience of Circumstellar Shells about B>=10 OH/IR Stars. I. Basic Statistics

Short title: Lewis (2000)
Authors: Lewis, B. M.
Journal: The Astrophysical Journal, Volume 533, Issue 2, pp. 959-968.
Bibcode: 2000ApJ...533..959L

Detection table from Lewis (2000)

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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
119 41 8.2+02 02 3140.5051-10.0855G40.505-10.086
IRAS 19386+0155166511.07.00.075ENG15-H2O +OH -SiO LEW00
220 55 17.7+29 20 4973.5337-10.1172G73.534-10.117
IRAS 20531+29091665141.0-141.00.018ENG15+OH LEW00
20 55 17.7+29 20 4973.5337-10.1172G73.534-10.117
IRAS 20531+29091667141.0-141.00.020ENG15+OH LEW00
20 55 17.7+29 20 4973.5337-10.1172G73.534-10.117
IRAS 20531+2909161210.0-142.00.410ENG15+OH LEW00
319 41 8.2+02 02 3140.5051-10.0855G40.505-10.086
IRAS 19386+0155166729.09.00.073ENG15-H2O +OH -SiO LEW00
19 41 8.2+02 02 3140.5051-10.0855G40.505-10.086
IRAS 19386+0155161226.014.00.058ENG15-H2O +OH -SiO LEW00
420 16 00+13 18 5554.8396-11.9662G54.840-11.966
IRAS 20136+1309166738.0-38.00.010ENG15+OH -SiO LEW00
519 13 58.6+00 07 3135.6196-4.9558G35.620-4.956
IRAS 19114+00021665109.0109.00.170ENG15-H2O +OH -SiO LEW00
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Non-detection table from Lewis (2000)

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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
120 16 00+13 18 5554.8396-11.9662G54.840-11.966
IRAS 20136+13090.005ENG15+OH -SiO LEW00
20 16 00+13 18 5554.8396-11.9662G54.840-11.966
IRAS 20136+13090.009ENG15+OH -SiO LEW00
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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

    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 LEW00

    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 LEW00 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