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POL10 - Class I Methanol Emission Around DR 21 (OH)

Short title: Polushkin & Valtts (2010)
Authors: Polushkin, S. V. Val'tts, I. E.
Journal: Astronomy Reports, Volume 54, Issue 6, pp.496-508
Bibcode: 2010ARep...54..496P

Detection table from Polushkin & Valtts (2010)

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ID Obs. RA Obs. Dec l b Group id Source name Other name Line Vpeak FWHM Fpeak ∫F dv Telescope Beam Detection Date
(J2000) (J2000) (deg.) (deg.) Comp CH3OH (class I) (km/s) (km/s) (Jy) (Jy*km/s) (arcsec) Yes/No
120 39 4.6+42 26 7.881.77230.5960G81.767+0.596
B9-1 h136 GHz (I)
-5.51.24.55.7ONSALA105+H2O +CH3OH I +CH3OH II +OH 2007-2008
20 39 4.6+42 26 7.881.77230.5960G81.767+0.596
B9-1 h236 GHz (I)
-4.30.83.93.3ONSALA105+H2O +CH3OH I +CH3OH II +OH 2007-2008
20 39 4.6+42 26 7.881.77230.5960G81.767+0.596
B9-1 h336 GHz (I)
-3.11.26.38ONSALA105+H2O +CH3OH I +CH3OH II +OH 2007-2008
20 39 4.6+42 26 7.881.77230.5960G81.767+0.596
B9-1 h436 GHz (I)
0.41.213.417ONSALA105+H2O +CH3OH I +CH3OH II +OH 2007-2008
220 39 0.2+42 23 0281.72310.5753G81.699+0.563
B6-1136 GHz (I)
-4.71.47.110.5ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 39 0.2+42 23 0281.72310.5753G81.699+0.563
B6-1236 GHz (I)
-3.51.14.55.2ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 39 0.2+42 23 0281.72310.5753G81.699+0.563
B6-1336 GHz (I)
-2.90.32.50.8ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 39 0.2+42 23 0281.72310.5753G81.699+0.563
B6-1436 GHz (I)
-1.93.36.422.4ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 39 0.2+42 23 0281.72310.5753G81.699+0.563
B6-1536 GHz (I)
0.10.88.47.1ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
320 38 58.3+42 21 0981.69460.5609G81.699+0.563
B4-1136 GHz (I)
-4.20.98.58.1ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 38 58.3+42 21 0981.69460.5609G81.699+0.563
B4-1236 GHz (I)
-3.30.68.95.7ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
420 38 59.9+42 20 5181.69360.5539G81.699+0.563
B3-1136 GHz (I)
-4.30.44.61.9ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 38 59.9+42 20 5181.69360.5539G81.699+0.563
B3-1236 GHz (I)
-3.514.44.7ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 38 59.9+42 20 5181.69360.5539G81.699+0.563
B3-1336 GHz (I)
-2.60.31.80.6ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
520 38 53.1+42 20 0881.67140.5633G81.699+0.563
B1-1 : B1-3136 GHz (I)
-2.80.79.57ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
620 38 54.8+42 19 21.881.66440.5514G81.699+0.563
DR 21West136 GHz (I)
-2.70.623.214.7ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 38 54.8+42 19 21.881.66440.5514G81.699+0.563
DR 21West236 GHz (I)
-1.61.25.67.1ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 38 54.8+42 19 21.881.66440.5514G81.699+0.563
DR 21West336 GHz (I)
-0.50.34.11.3ONSALA105+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
720 39 4.6+42 26 7.881.77230.5960G81.767+0.596
B 9-1 h144 GHz (I)
-4.70.534.219.6ONSALA88+H2O +CH3OH I +CH3OH II +OH 2007-2008
20 39 4.6+42 26 7.881.77230.5960G81.767+0.596
B 9-1 h244 GHz (I)
-3.90.5116ONSALA88+H2O +CH3OH I +CH3OH II +OH 2007-2008
20 39 4.6+42 26 7.881.77230.5960G81.767+0.596
B 9-1 h344 GHz (I)
-3.50.372.6ONSALA88+H2O +CH3OH I +CH3OH II +OH 2007-2008
20 39 4.6+42 26 7.881.77230.5960G81.767+0.596
B 9-1 h444 GHz (I)
-2.50.514.67.9ONSALA88+H2O +CH3OH I +CH3OH II +OH 2007-2008
820 39 02+42 25 4381.76200.5981G81.767+0.596
DR21N144 GHz (I)
-4.60.335.210.5ONSALA88+H2O +CH3OH I +CH3OH II +OH 2007-2008
20 39 02+42 25 4381.76200.5981G81.767+0.596
DR21N244 GHz (I)
-3.60.220.5ONSALA88+H2O +CH3OH I +CH3OH II +OH 2007-2008
20 39 02+42 25 4381.76200.5981G81.767+0.596
DR21N44 GHz (I)
-2.60.47.32.4ONSALA88+H2O +CH3OH I +CH3OH II +OH 2007-2008
920 39 0.2+42 23 0281.72310.5753G81.699+0.563
B6-3144 GHz (I)
0.10.98.78.3ONSALA88+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 39 0.2+42 23 0281.72310.5753G81.699+0.563
B6-3244 GHz (I)
1.20.310.32.2ONSALA88+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
1020 39 0.2+42 23 0281.72310.5753G81.699+0.563
B 6-1144 GHz (I)
0.40.614793.4ONSALA88+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 39 0.2+42 23 0281.72310.5753G81.699+0.563
B 6-1244 GHz (I)
0.90.410142.8ONSALA88+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
1120 39 2.2+42 22 43.981.72290.5673G81.699+0.563
DR 21(OH)144 GHz (I)
0.40.6212.2135ONSALA88+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 39 2.2+42 22 43.981.72290.5673G81.699+0.563
DR 21(OH)244 GHz (I)
0.90.4150.463.7ONSALA88+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
1220 38 58.3+42 21 0981.69460.5609G81.699+0.563
B4-1144 GHz (I)
-40.77.15.2ONSALA88+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 38 58.3+42 21 0981.69460.5609G81.699+0.563
B4-1244 GHz (I)
-20.711.18.2ONSALA88+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
20 38 58.3+42 21 0981.69460.5609G81.699+0.563
B4-1344 GHz (I)
0.60.98.17.7ONSALA88+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
1320 38 53.1+42 20 0881.67140.5633G81.699+0.563
B 1-1 : B 1-3144 GHz (I)
-20.816.113.6ONSALA88+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
1420 38 54.8+42 19 21.881.66440.5514G81.699+0.563
DR 21 West144 GHz (I)
-2.10.517492.2ONSALA88+H2O +CH3OH I +CH3OH II +OH -SiO 2007-2008
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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

    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 POL10

    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 POL10 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