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Data: H2O, SiO

NAK00 - Detections of SiO and H_2O Masers in the Bipolar Nebula IRAS 19312+1950

  Interferometry data

Short title: Nakashima & Deguchi (2000)
Authors: Nakashima, Jun-ichi Deguchi, Shuji
Journal: Publications of the Astronomical Society of Japan, v.52, p.L43-L46.
Bibcode: 2000PASJ...52L..43N

PDF: NAK00.pdf

Detection table from Nakashima & Deguchi (2000)

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ID Obs. RA Obs. Dec l b Source name Line Vpeak Ta ∫Ta dv Date Telescope RMS List Ref.
(J2000) (J2000) (deg.) (deg.) SiO (km/s) (K) (K*km/s) (Jy)
119 33 24.2+19 56 5555.3704840.185604IRAS 19312+195025.52000-05-30ENG_SIONAK00
219 33 24.3+19 56 54.955.3707160.185107IRAS19312+1950SiO J=1-0 v=1
25.540.1130.6072000-05-30NRO0.027NRONAK00
319 33 24.3+19 56 54.955.3707160.185107IRAS19312+1950SiO J=1-0 v=2
26.840.1180.3572000-05-30NRO0.022NRONAK00
419 33 24.3+19 56 54.955.3707160.185107IRAS19312+1950SiO J=2-1 v=1
17.440.2851.9622000-05-25NRO0.015NRONAK00
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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 NAK00

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

  • Distribution of sources from NAK00 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