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Reference: [ETO04B]

Detection table from ETO04B

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ID Obs. RA Obs. Dec l b Group id Source name Frequency Vrange Vpeak Fpeak List Detection Class Dist. (parallax) Ref.
(J2000) (J2000) (deg.) (deg.) (MHz) (km/s) (km/s) (Jy) Yes/No (kpc)
122 19 27.8+59 51 22104.90892.4131G104.908+2.413
IRAS 22177+5936166729.2-40.00.420ENG15+H2O +OH +SiO EVOLVEDETO04B
219 27 41.6+16 37 2251.8025-0.2236G51.804-0.224
IRAS 19254+1631166737.1-17.10.140ENG15+H2O -CH3OH II +OH +SiO EVOLVEDETO04B
318 51 25.7-01 03 5531.9827-0.4836G31.984-0.485
IRAS 18488-0107166741.655.20.160ENG15+H2O -CH3OH II +OH +SiO EVOLVEDETO04B
419 08 58.3+08 37 4742.60340.0669G42.604+0.066
IRAS 19065+0832166734.336.00.470ENG15+H2O -CH3OH II +OH +SiO SFR_MIXEDETO04B
518 48 40.3-02 50 3530.0864-0.6812G30.091-0.686
IRAS 18460-0254166742.677.71.940ENG15+H2O -CH3OH II +OH +SiO SFR_MIXEDETO04B
618 45 52.7-01 46 4330.71520.4254G30.715+0.427
IRAS 18432-0149166734.349.80.590ENG15+H2O -CH3OH II +OH +SiO SFR_MIXEDETO04B
718 28 28.5-09 58 1821.45110.4996G21.457+0.491
IRAS 18257-1000166736.595.92.520ENG15+H2O +OH +SiO EVOLVEDETO04B
818 22 42.2-12 47 4418.29340.4321G18.296+0.429
IRAS 18198-1249166730.932.80.550ENG15-H2O +OH +SiO EVOLVEDETO04B
918 16 26-14 55 1315.70170.7699G15.701+0.770
IRAS 18135-1456166728.7-13.40.910ENG15+H2O -CH3OH I -CH3OH II +OH +SiO EVOLVEDETO04B
1017 58 4.1-21 21 097.95911.4474G7.961+1.445
IRAS 17550-2120166726.9-34.90.940ENG15-H2O -CH3OH I +OH EVOLVEDETO04B
1117 44 58.6-27 14 451.36831.0026G1.368+1.003
IRAS 17418-2713166733.2-29.33.720ENG15+OH EVOLVEDETO04B
1217 42 31.7-33 21 00355.8927-1.7478G355.893-1.748
IRAS 17392-3319166728.6-59.00.270ENG15+OH EVOLVEDETO04B
1317 44 22.6-31 55 39357.3085-1.3330G357.308-1.333
IRAS 17411-3154166737.1-41.118.870ENG15-H2O +OH +SiO EVOLVEDETO04B
1417 35 2.1-33 33 30354.8825-0.5370G354.884-0.538
IRAS 17317-3331166729.2-4.00.810ENG15+H2O +OH +SiO EVOLVEDETO04B
1519 26 47.6+11 21 1547.0634-2.5393G47.063-2.540
IRAS 19244+1115166735.463.90.580ENG15-H2O +OH -SiO EVOLVEDETO04B
1619 18 14.5+23 49 2657.12405.1166G57.124+5.116
IRAS 19161+2343166738.210.00.570ENG15+H2O -CH3OH II +OH +SiO EVOLVEDETO04B
1719 09 57.1+09 26 5243.44080.2296G43.441+0.229
IRAS 19075+0921166714.05.30.700ENG15+H2O +OH -SiO SFR_MIXEDETO04B
1817 53 46.5-31 44 26358.4956-2.9492G358.496-2.949
IRAS 17505-3143166733.2-12.90.380ENG15+OH +SiO EVOLVEDETO04B
1922 54 31.9+60 49 38109.16061.1203G109.160+1.121
IRAS 22525+6033166719.1-62.10.170ENG15+H2O +OH +SiO EVOLVEDETO04B
2017 51 26.5-28 25 361.0952-0.8310G1.095-0.831
IRAS 17482-2824166742.7-10.80.430ENG15+OH +SiO EVOLVEDETO04B
2120 42 18.7-08 15 3238.2823-28.3701G38.283-28.370
IRAS 20396-082616676.2-53.40.070ENG15+OH +SiO EVOLVEDETO04B
2219 21 26.3+11 33 5446.6293-1.2832G46.629-1.284
IRAS 19190+1128166733.241.10.180ENG15+OH +SiO EVOLVEDETO04B
2318 37 32.2-05 23 5926.54300.6188G26.543+0.618
IRAS 18348-0526166725.813.89.270ENG15+H2O +OH +SiO EVOLVEDETO04B
2415 28 43.7+03 49 438.103545.8400G8.104+45.840
IRAS 15262+0400166712.437.80.300ENG15+H2O +OH +SiO EVOLVEDETO04B
2522 19 27.8+59 51 22104.90892.4131G104.908+2.413
IRAS 22177+5936166529.8-41.20.140ENG15+H2O +OH +SiO EVOLVEDETO04B
2619 37 23.5+20 36 5556.4080-0.3071G56.409-0.308
IRAS 19352+203016651.4-1.40.470ENG15+H2O -CH3OH II +OH -SiO EVOLVEDETO04B
2719 09 57.1+09 26 5243.44080.2296G43.441+0.229
IRAS 19075+0921166515.85.20.460ENG15+H2O +OH -SiO SFR_MIXEDETO04B
2819 26 47.6+11 21 1547.0634-2.5393G47.063-2.540
IRAS 19244+1115166542.756.62.990ENG15-H2O +OH -SiO EVOLVEDETO04B
2917 35 2.1-33 33 30354.8825-0.5370G354.884-0.538
IRAS 17317-3331166531.5-6.30.160ENG15+H2O +OH +SiO EVOLVEDETO04B
3017 41 52-33 33 40355.6405-1.7416G355.640-1.742
IRAS 17385-3332166532.7-258.20.140ENG15-H2O +OH EVOLVEDETO04B
3117 42 31.7-33 21 00355.8927-1.7478G355.893-1.748
IRAS 17392-3319166537.7-60.20.080ENG15+OH EVOLVEDETO04B
3219 08 58.3+08 37 4742.60340.0669G42.604+0.066
IRAS 19065+0832166534.934.90.140ENG15+H2O -CH3OH II +OH +SiO SFR_MIXEDETO04B
3319 37 23.5+20 36 5556.4080-0.3071G56.409-0.308
IRAS 19352+203016671.4-1.40.750ENG15+H2O -CH3OH II +OH -SiO EVOLVEDETO04B
3418 48 40.3-02 50 3530.0864-0.6812G30.091-0.686
IRAS 18460-0254166581.081.00.100ENG15+H2O -CH3OH II +OH +SiO SFR_MIXEDETO04B
3518 45 52.7-01 46 4330.71520.4254G30.715+0.427
IRAS 18432-0149166534.348.70.140ENG15+H2O -CH3OH II +OH +SiO SFR_MIXEDETO04B
3615 28 43.7+03 49 438.103545.8400G8.104+45.840
IRAS 15262+0400166510.738.40.190ENG15+H2O +OH +SiO EVOLVEDETO04B
3720 42 18.7-08 15 3238.2823-28.3701G38.283-28.370
IRAS 20396-0826166551.1-51.10.160ENG15+OH +SiO EVOLVEDETO04B
3818 37 32.2-05 23 5926.54300.6188G26.543+0.618
IRAS 18348-0526166529.212.12.360ENG15+H2O +OH +SiO EVOLVEDETO04B
3918 16 26-14 55 1315.70170.7699G15.701+0.770
IRAS 18135-1456166529.3-16.20.160ENG15+H2O -CH3OH I -CH3OH II +OH +SiO EVOLVEDETO04B
4017 44 58.6-27 14 451.36831.0026G1.368+1.003
IRAS 17418-2713166521.4-21.40.340ENG15+OH EVOLVEDETO04B
4117 58 4.1-21 21 097.95911.4474G7.961+1.445
IRAS 17550-2120166527.5-34.90.500ENG15-H2O -CH3OH I +OH EVOLVEDETO04B
4217 44 22.6-31 55 39357.3085-1.3330G357.308-1.333
IRAS 17411-3154166524.2-38.30.320ENG15-H2O +OH +SiO EVOLVEDETO04B
4318 28 28.5-09 58 1821.45110.4996G21.457+0.491
IRAS 18257-1000166595.995.90.170ENG15+H2O +OH +SiO EVOLVEDETO04B
4422 54 31.9+60 49 38109.16061.1203G109.160+1.121
IRAS 22525+6033166520.8-62.70.410ENG15+H2O +OH +SiO EVOLVEDETO04B
4517 51 26.5-28 25 361.0952-0.8310G1.095-0.831
IRAS 17482-2824166541.6-10.80.120ENG15+OH +SiO EVOLVEDETO04B
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Non-detection table from ETO04B

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ID Obs. RA Obs. Dec l b Group id Source name Line Fpeak List Detection Class Ref.
(J2000) (J2000) (deg.) (deg.) OH (Jy) Yes/No
115 25 47.7-36 13 56334.666316.9547G334.666+16.955
IRAS 15226-36031.665 GHz; 0.120ENG15+OH +SiO EVOLVEDETO04B
218 06 22.5-21 11 289.0551-0.1557G9.055-0.156
IRAS 18033-21111.667 GHz; 0.120ENG15+OH EVOLVEDETO04B
317 41 52-33 33 40355.6405-1.7416G355.640-1.742
IRAS 17385-33321.667 GHz; ENG15-H2O +OH EVOLVEDETO04B
420 57 16.3+02 58 4651.3639-26.1127G51.364-26.113
IRAS 20547+02471.667 GHz; ENG15+H2O -CH3OH II +OH -SiO EVOLVEDETO04B
517 25 7.1-24 51 030.98376.0500G0.984+6.050
IRAS 17220-24481.667 GHz; 0.120ENG15-CH3OH II +OH EVOLVEDETO04B
615 25 47.7-36 13 56334.666316.9547G334.666+16.955
IRAS 15226-36031.667 GHz; 0.120ENG15+OH +SiO EVOLVEDETO04B
719 27 41.6+16 37 2251.8025-0.2236G51.804-0.224
IRAS 19254+16311.665 GHz; 0.120ENG15+H2O -CH3OH II +OH +SiO EVOLVEDETO04B
817 53 46.5-31 44 26358.4956-2.9492G358.496-2.949
IRAS 17505-31431.665 GHz; 0.120ENG15+OH +SiO EVOLVEDETO04B
919 18 14.5+23 49 2657.12405.1166G57.124+5.116
IRAS 19161+23431.665 GHz; ENG15+H2O -CH3OH II +OH +SiO EVOLVEDETO04B
1019 21 26.3+11 33 5446.6293-1.2832G46.629-1.284
IRAS 19190+11281.665 GHz; 0.120ENG15+OH +SiO EVOLVEDETO04B
1117 25 7.1-24 51 030.98376.0500G0.984+6.050
IRAS 17220-24481.665 GHz; ENG15-CH3OH II +OH EVOLVEDETO04B
1218 51 25.7-01 03 5531.9827-0.4836G31.984-0.485
IRAS 18488-01071.665 GHz; 0.120ENG15+H2O -CH3OH II +OH +SiO EVOLVEDETO04B
1320 57 16.3+02 58 4651.3639-26.1127G51.364-26.113
IRAS 20547+02471.665 GHz; ENG15+H2O -CH3OH II +OH -SiO EVOLVEDETO04B
1418 06 22.5-21 11 289.0551-0.1557G9.055-0.156
IRAS 18033-21111.665 GHz; 0.120ENG15+OH EVOLVEDETO04B
1518 22 42.2-12 47 4418.29340.4321G18.296+0.429
IRAS 18198-12491.665 GHz; 0.120ENG15-H2O +OH +SiO EVOLVEDETO04B
×
  • Distribution of sources in all sky (l,b)

    0

  • Distribution of sources in all sky using Aladin

    Tip: Click on some source to get more informaiton


  • 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 ETO04B

    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 ETO04B 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

    Download UKIDSS K FITS
    2MASS K

    Download 2MASS K FITS