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Select data type: CH3OH_I

HAS89 - The detection of the 4(-1)-3(0) E transition of methanol at 36.2 GHz toward hot H II regions

Short title: Haschick & Baan (1989)
Authors: Haschick, Aubrey D. Baan, Willem A.
Journal: Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 339, April 15, 1989, p. 949-955.
Bibcode: 1989ApJ...339..949H

PDF: HAS89.pdf

Detection table from Haschick & Baan (1989)

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ID Obs. RA Obs. Dec l b Group id Other name Line Vpeak FWHM List Beam Detection Ref.
(J2000) (J2000) (deg.) (deg.) Comp CH3OH (class I) (km/s) (km/s) (arcsec) Yes/No
120 39 0.7+42 22 50.881.72160.5722G81.722+0.572
36 GHz (I)
0.40.56AVE0260+CH3OH I +CH3OH II +OH -SiO HAS89
20 39 0.7+42 22 50.881.72160.5722G81.722+0.572
36 GHz (I)
-3.33.9AVE0260+CH3OH I +CH3OH II +OH -SiO HAS89
220 10 9.1+31 31 37.469.5406-0.9756G69.540-0.976
36 GHz (I)
11.02.4AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
317 45 38.2-29 05 45.5359.8654-0.0863G359.985-0.050
36 GHz (I)
11.57.4AVE0260+H2O +CH3OH I +CH3OH II +OH +SiO HAS89
17 45 38.2-29 05 45.5359.8654-0.0863G359.985-0.050
36 GHz (I)
2.89.3AVE0260+H2O +CH3OH I +CH3OH II +OH +SiO HAS89
406 08 54.2+21 38 36.6188.94600.8900G188.946+0.887
36 GHz (I)
3.52.6AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
518 14 39.8-17 51 58.312.9095-0.2610G12.908-0.260
36 GHz (I)
36.24.6AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
619 11 54.3+09 35 55.443.7972-0.1276G43.795-0.127
36 GHz (I)
43.04.7AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
720 01 46.3+01 17 36.142.3337-14.9812G42.334-14.981
36 GHz (I)
44.27.3AVE0260+CH3OH I HAS89
819 23 53.9+14 30 37.149.5094-0.4225G49.509-0.422
36 GHz (I)
55.26.8AVE0260+CH3OH I HAS89
918 53 18.6+01 14 57.734.25720.1532G34.257+0.153
36 GHz (I)
57.85.1AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
1019 23 43.8+14 31 6.449.4974-0.3831G49.488-0.387
36 GHz (I)
59.82.8AVE0260+H2O +CH3OH I +CH3OH II +OH -SiO HAS89
1106 41 12.8+09 29 18.7203.32532.0641G203.316+2.055
36 GHz (I)
7.30.6AVE0260+H2O +CH3OH I +CH3OH II HAS89
06 41 12.8+09 29 18.7203.32532.0641G203.316+2.055
36 GHz (I)
8.55.1AVE0260+H2O +CH3OH I +CH3OH II HAS89
06 41 12.8+09 29 18.7203.32532.0641G203.316+2.055
36 GHz (I)
7.53.6AVE0260+H2O +CH3OH I +CH3OH II HAS89
1217 47 20.4-28 23 7.30.6667-0.0363G0.667-0.036
I36 GHz (I)
70.46.8AVE0260+H2O +CH3OH I +CH3OH II +OH +SiO HAS89
17 47 20.4-28 23 7.30.6667-0.0363G0.667-0.036
I36 GHz (I)
62.622.4AVE0260+H2O +CH3OH I +CH3OH II +OH +SiO HAS89
1320 38 36.8+42 37 37.581.87260.7801G81.877+0.783
(N)36 GHz (I)
9.52.9AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
1418 47 47-01 54 35.130.8157-0.0580G30.817-0.057
36 GHz (I)
98.55.5AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
1505 40 53.3+35 41 48.8173.71882.6980G173.719+2.698
36 GHz (I)
-16.60.9AVE0260+H2O +CH3OH I +CH3OH II -OH HAS89
1602 27 4.7+61 52 25.5133.94881.0651G133.948+1.064
36 GHz (I)
-46.52.1AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
1723 13 44.8+61 26 53.7111.53330.7575G111.542+0.766
36 GHz (I)
-55.92.8AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
1823 13 45.4+61 28 9.7111.54220.7767G111.542+0.766
36 GHz (I)
-57.43.7AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
1918 10 28.5-19 55 49.110.6232-0.3830G10.623-0.383
36 GHz (I)
-61.0AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
2017 20 53.4-35 47 1.5351.41700.6450G351.417+0.645
36 GHz (I)
-8.73.8AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
17 20 53.4-35 47 1.5351.41700.6450G351.417+0.645
36 GHz (I)
-4.62.1AVE0260+H2O +CH3OH I +CH3OH II +OH HAS89
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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 HAS89

    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 HAS89 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