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SIV99 - Overshoot of main-line spectral extent in circumstellar OH masers

Short title: Sivagnanam & David (1999)
Authors: Sivagnanam, P. David, P.
Journal: Monthly Notices of the Royal Astronomical Society, Volume 304, Issue 3, pp. 622-632.
Bibcode: 1999MNRAS.304..622S

Detection table from Sivagnanam & David (1999)

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ID Obs. RA Obs. Dec l b Group id Source name Frequency Vrange Vpeak List Detection Ref.
(J2000) (J2000) (deg.) (deg.) (MHz) (km/s) (km/s) Yes/No
117 25 7.1-24 51 030.98376.0500G0.984+6.050
IRAS 17220-2448161220.320.3ENG15-CH3OH II +OH SIV99
217 32 34.6-29 43 16357.82031.9869G357.820+1.987
IRAS 17293-2941161229.5-45.4ENG15+OH SIV99
317 34 57.9-35 25 53353.2990-1.5380G353.299-1.538
IRAS 17316-3523166747.147.1ENG15+OH SIV99
17 34 57.9-35 25 53353.2990-1.5380G353.299-1.538
IRAS 17316-3523161225.249.1ENG15+OH SIV99
417 42 31.7-33 21 00355.8927-1.7478G355.893-1.748
IRAS 17392-3319166728.9-59.3ENG15+OH SIV99
17 42 31.7-33 21 00355.8927-1.7478G355.893-1.748
IRAS 17392-3319161227.0-57.5ENG15+OH SIV99
517 44 51-31 32 29357.6904-1.2171G357.690-1.217
IRAS 17416-3131161260.660.6ENG15+OH SIV99
617 53 46.9-33 13 24357.2139-3.6985G357.214-3.698
IRAS 17504-3312161231.1-78.3ENG15+OH SIV99
718 10 53.7-26 13 305.1482-3.4972G5.148-3.497
IRAS 18077-2614161228.585.9ENG15+OH +SiO SIV99
818 12 19.2-23 47 007.4495-2.6111G7.450-2.611
IRAS 18092-2347166736.929.1ENG15-H2O +OH SIV99
18 12 19.2-23 47 007.4495-2.6111G7.450-2.611
IRAS 18092-2347161235.930.8ENG15-H2O +OH SIV99
918 16 26-14 55 1315.70170.7699G15.701+0.770
IRAS 18135-1456166731.2-16.0ENG15+H2O -CH3OH I -CH3OH II +OH +SiO SIV99
18 16 26-14 55 1315.70170.7699G15.701+0.770
IRAS 18135-1456161228.4-15.3ENG15+H2O -CH3OH I -CH3OH II +OH +SiO SIV99
1018 28 28.5-09 58 1821.45110.4996G21.457+0.491
IRAS 18257-1000166736.595.9ENG15+H2O +OH +SiO SIV99
18 28 28.5-09 58 1821.45110.4996G21.457+0.491
IRAS 18257-1000161236.497.8ENG15+H2O +OH +SiO SIV99
1118 28 59.4-07 33 2523.64941.5076G23.649+1.508
IRAS 18262-0735161227.764.9ENG15+OH SIV99
1218 30 32.7-10 57 3220.8125-0.4091G20.812-0.409
IRAS 18277-1059166736.684.8ENG15+OH SIV99
18 30 32.7-10 57 3220.8125-0.4091G20.812-0.409
IRAS 18277-1059161236.085.3ENG15+OH SIV99
1318 32 50.5-21 09 3711.9895-5.5853G11.989-5.585
IRAS 18298-2111166724.984.5ENG15-H2O -CH3OH II +OH SIV99
18 32 50.5-21 09 3711.9895-5.5853G11.989-5.585
IRAS 18298-2111161224.086.2ENG15-H2O -CH3OH II +OH SIV99
1418 45 52.7-01 46 4330.71520.4254G30.715+0.427
IRAS 18432-0149166735.848.6ENG15+H2O +OH +SiO SIV99
18 45 52.7-01 46 4330.71520.4254G30.715+0.427
IRAS 18432-0149161235.049.0ENG15+H2O +OH +SiO SIV99
1518 48 40.3-02 50 3530.0864-0.6812G30.091-0.686
IRAS 18460-0254166743.377.2ENG15+H2O +OH +SiO SIV99
18 48 40.3-02 50 3530.0864-0.6812G30.091-0.686
IRAS 18460-0254161240.978.6ENG15+H2O +OH +SiO SIV99
1619 18 14.5+23 49 2657.12405.1166G57.124+5.116
IRAS 19161+2343166738.210.2ENG15+H2O -CH3OH II +OH +SiO SIV99
19 18 14.5+23 49 2657.12405.1166G57.124+5.116
IRAS 19161+2343161235.910.7ENG15+H2O -CH3OH II +OH +SiO SIV99
1719 27 41.6+16 37 2251.8025-0.2236G51.804-0.225
IRAS 19254+1631161237.4-17.3ENG15+H2O +OH +SiO SIV99
1820 04 20.4+29 04 0566.7929-1.2464G66.794-1.247
IRAS 20023+2855166727.2-78.9ENG15-H2O +OH +SiO SIV99
20 04 20.4+29 04 0566.7929-1.2464G66.794-1.247
IRAS 20023+2855161223.9-77.1ENG15-H2O +OH +SiO SIV99
1920 10 27.4-06 16 1636.3564-20.4151G36.357-20.415
IRAS 20077-0625166728.0-30.9ENG15-H2O -CH3OH II +OH +SiO SIV99
20 10 27.4-06 16 1636.3564-20.4151G36.357-20.415
IRAS 20077-0625161224.0-31.4ENG15-H2O -CH3OH II +OH +SiO SIV99
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Non-detection table from Sivagnanam & David (1999)

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ID Obs. RA Obs. Dec l b Group id Source name List Detection Ref.
(J2000) (J2000) (deg.) (deg.) Yes/No
103 31 3.8-15 24 52203.6891-51.2008G203.689-51.201
IRAS 03287-1535ENG15+H2O +OH -SiO SIV99
03 31 3.8-15 24 52203.6891-51.2008G203.689-51.201
IRAS 03287-1535ENG15+H2O +OH -SiO SIV99
217 25 7.1-24 51 030.98376.0500G0.984+6.050
IRAS 17220-2448ENG15-CH3OH II +OH SIV99
317 32 34.6-29 43 16357.82031.9869G357.820+1.987
IRAS 17293-2941ENG15+OH SIV99
417 39 52-27 23 360.64511.8900G0.645+1.890
IRAS 17367-2722ENG15+OH SIV99
17 39 52-27 23 360.64511.8900G0.645+1.890
IRAS 17367-2722ENG15+OH SIV99
517 44 51-31 32 29357.6904-1.2171G357.690-1.217
IRAS 17416-3131ENG15+OH SIV99
617 53 46.9-33 13 24357.2139-3.6985G357.214-3.698
IRAS 17504-3312ENG15+OH SIV99
718 10 53.7-26 13 305.1482-3.4972G5.148-3.497
IRAS 18077-2614ENG15+OH +SiO SIV99
818 28 59.4-07 33 2523.64941.5076G23.649+1.508
IRAS 18262-0735ENG15+OH SIV99
919 27 41.6+16 37 2251.8025-0.2236G51.804-0.225
IRAS 19254+1631ENG15+H2O +OH +SiO SIV99
×
  • 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 SIV99

    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 SIV99 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