Display data from paper

Data: H2O

NAKA93 - Detection of SiO and H2O masers in Galactic bulge sources

Short title: Nakada et al. (1993)
Authors: Nakada, Yoshikazu Onaka, Takashi Yamamura, Issei Deguchi, Shuji Ukita, Nobuharu Izumiura, Hideyuki
Journal: PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 45, no. 2, p. 179-189.
Bibcode: 1993PASJ...45..179N

PDF: NAKA93.pdf

Detection table from Nakada et al. (1993)

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ID Obs. RA Obs. Dec l b Group id Source name Vrange Vlow Vup Vpeak Fpeak Date RMS Detection
(J2000) (J2000) (deg.) (deg.) (km/s) (km/s) (km/s) (km/s) (Jy) (Jy) Yes/No
117 18 37.4-25 50 02359.33676.7138G359.337+6.714
IRAS 17155-2546 -46.60.6721990-01-230.170+H2O +OH +SiO
217 22 23.4-27 20 07358.56905.1710G358.569+5.171
IRAS 17192-2717 32.6-171.6-139.0-171.61.8481990-01-230.170+H2O -OH +SiO
317 28 11.1-26 17 420.15864.6756G0.159+4.675
IRAS 17250-2615 -16.21.0921990-01-230.170+H2O -OH +SiO
417 42 40.2-21 24 106.08214.5034G6.082+4.503
IRAS 17396-2122 21.80.7841990-01-230.170+H2O -OH +SiO
517 45 12.4-23 08 274.90173.0970G4.902+3.097
IRAS 17421-2307 24.23.2481990-01-230.170+H2O -OH +SiO
618 10 38.7-28 05 043.4849-4.3381G3.485-4.338
IRAS 18074-2805 110.50.421990-01-230.170+H2O -OH +SiO
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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

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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 NAKA93

    Tip: Use "Box select" or "Lasso select" to display velocity-selected sources in Aladin all-sky view

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

  • Distribution of sources from NAKA93 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