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TAN97 - The relation between water maser and CO outflow in strong far infrared sources

Short title: Tang et al. (1997)
Authors: Tang, Ge-shi Sun, Jin Lu, Jing
Journal: Chinese Astronomy and Astrophysics, Volume 21, Issue 2, p. 197-211.
Bibcode: 1997ChA&A..21..197T

Detection table from Tang et al. (1997)

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ID Obs. RA Obs. Dec l b Group id Source name Image Line Vrange Vpeak Fpeak Telescope Vstep RMS Beam Detection Class Dist. (parallax) Date
(J2000) (J2000) (deg.) (deg.) H2O (km/s) (km/s) (Jy) (km/s) (Jy) (arcsec) Yes/No (kpc)
102 26 50.8+62 15 52.2133.78271.4198G133.783+1.420
02230+6202 Image 22 GHz; -46;-45.2-4679.3PMODLH0.1638.800250+H2O -CH3OH I -CH3OH II SFR93 5 20
02 26 50.8+62 15 52.2133.78271.4198G133.783+1.420
02230+620222 GHz; -46.2;-45.3-46.223.9PMODLH0.165.730250+H2O -CH3OH I -CH3OH II SFR93 12 1
306 09 7.8+21 50 38.7188.79591.0331G188.796+1.033
06061+2151 Image 22 GHz; -5.7;-14.5-5.794.2PMODLH0.1623.300250+H2O -CH3OH I +CH3OH II SFR93 5 21
406 09 51.7+20 29 25.4190.06330.5275G190.054+0.533
06068+2030 Image 22 GHz; -40.132.3PMODLH0.1611.400250+H2O -CH3OH I -CH3OH II SFR_MIXED93 8 16
06 09 51.7+20 29 25.4190.06330.5275G190.054+0.533
06068+203022 GHz; -38.728.5PMODLH0.168.550250+H2O -CH3OH I -CH3OH II SFR_MIXED93 12 4
609 47 56.7+13 16 42.9221.445145.0577G221.445+45.058
09452+1330 Image 22 GHz; -21.2;-18.8-21.275.5PMODLH0.1616.800250+H2O -CH3OH I -OH EVOLVED93 5 17
09 47 56.7+13 16 42.9221.445145.0577G221.445+45.058
09452+133022 GHz; -30.3;-31.5-30.337.3PMODLH0.169.310250+H2O -CH3OH I -OH EVOLVED93 8 16
09 47 56.7+13 16 42.9221.445145.0577G221.445+45.058
09452+133022 GHz; -21.620.5PMODLH0.165.890250+H2O -CH3OH I -OH EVOLVED93 12 5
918 27 38.7-03 49 54.126.79973.5287G26.802+3.526
18250-0351 Image 22 GHz; -75.522.5PMODLH0.164.550250+H2O -CH3OH I -CH3OH II -SiO SFR_MIXED93 8 14
1018 34 19.8-05 59 44.225.64691.0534G25.649+1.050
18316-0602 Image 22 GHz; 3988.2PMODLH0.1611.500250+H2O +CH3OH I +CH3OH II +OH SFR93 8 14
1118 42 58.2-04 13 59.828.1999-0.0499G28.200-0.050
18403-0417 Image 22 GHz; -19.1;-15.5-19.125.2PMODLH0.165.220250+H2O +CH3OH I +CH3OH II +OH SFR93 8 14
1219 00 59.3+04 12 6.437.7593-0.2043G37.763-0.214
18585+0407 Image 22 GHz; -62.522.9PMODLH0.165.700250+H2O +CH3OH I +CH3OH II SFR93 8 14
1319 13 27.8+10 53 33.945.12160.1321G45.122+0.132
19111+1048 Image 22 GHz; -4.7320.9PMODLH0.165.460250+H2O -CH3OH I +CH3OH II +OH SFR93 8 14
1420 10 11.5+27 29 6.466.1533-3.1846G66.153-3.185
20081+2720 Image 22 GHz; 42;33.84216.5PMODLH0.165.240250+H2O -CH3OH I -CH3OH II SFR93 8 14
1520 19 39.3+40 56 30.478.43602.6580G78.436+2.658
20178+4046 Image 22 GHz; -37.4;-46.1-37.416.9PMODLH0.164.900250+H2O -CH3OH I -CH3OH II -OH SFR_MIXED93 8 14
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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 TAN97

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

  • Distribution of sources from TAN97 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

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    2MASS K

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