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HAS90 - Detection of widespread strong methanol masers at 44 GHz

Short title: Haschick et al. (1990)
Authors: Haschick, Aubrey D. Menten, Karl M. Baan, Willem A.
Journal: Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 354, May 10, 1990, p. 556-567.
Bibcode: 1990ApJ...354..556H

Detection table from Haschick et al. (1990)

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ID Obs. RA Obs. Dec l b Group id Other name Line Vpeak FWHM ∫F dv List Beam Detection Class Dist. (parallax) Ref.
(J2000) (J2000) (deg.) (deg.) Comp CH3OH (class I) (km/s) (km/s) (Jy*km/s) (arcsec) Yes/No (kpc)
106 12 56.4+17 59 53.8192.5974-0.0355G192.599-0.048
44 GHz (I); 11.180.5717.00AVE0250+H2O +CH3OH I +CH3OH II SFR_MIXEDHAS90
220 10 9.1+31 31 37.469.5406-0.9756G69.540-0.976
44 GHz (I); 11.420.4911.70AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
20 10 9.1+31 31 37.469.5406-0.9756G69.540-0.976
44 GHz (I); 12.040.2811.70AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
419 10 13.4+09 06 14.443.16680.0114G43.167+0.011
44 GHz (I); 14.04.143.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFR_MIXEDHAS90
19 10 13.4+09 06 14.443.16680.0114G43.167+0.011
44 GHz (I); 15.570.4843.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFR_MIXEDHAS90
617 45 38.2-29 03 27.7359.8982-0.0664G359.8928-0.0671
44 GHz (I); 2114200.00AVE0250+H2O +CH3OH I +CH3OH II SFR_MIXEDHAS90
718 14 11.1-17 55 57.412.7968-0.1928G12.797-0.193
W33Met44 GHz (I); 32.640.6376.00AVE0250+H2O +CH3OH I +CH3OH II SFRHAS90
18 14 11.1-17 55 57.412.7968-0.1928G12.797-0.193
W33Met44 GHz (I); 36.281.376.00AVE0250+H2O +CH3OH I +CH3OH II SFRHAS90
918 06 19.3-21 37 37.98.6684-0.3576G8.669-0.357
44 GHz (I); 33.921.5108.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
18 06 19.3-21 37 37.98.6684-0.3576G8.669-0.357
44 GHz (I); 35.711.3108.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
18 06 19.3-21 37 37.98.6684-0.3576G8.669-0.357
44 GHz (I); 37.731.2108.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
18 06 19.3-21 37 37.98.6684-0.3576G8.669-0.357
44 GHz (I); 35.711.368.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
1318 14 11.1-17 55 57.412.7968-0.1928G12.797-0.193
44 GHz (I); 36.281.329.00AVE0250+H2O +CH3OH I +CH3OH II SFRHAS90
1418 06 19.3-21 37 37.98.6684-0.3576G8.669-0.357
44 GHz (I); 37.731.221.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
1517 45 52-28 59 26.7359.9815-0.0745G359.9815-0.0745
44 GHz (I); 44.512.5332.00AVE0250+CH3OH I +CH3OH II SFR_MIXEDHAS90
17 45 52-28 59 26.7359.9815-0.0745G359.9815-0.0745
44 GHz (I); 47.190.42332.00AVE0250+CH3OH I +CH3OH II SFR_MIXEDHAS90
17 45 52-28 59 26.7359.9815-0.0745G359.9815-0.0745
44 GHz (I); 47.190.4220.00AVE0250+CH3OH I +CH3OH II SFR_MIXEDHAS90
1819 23 43.9+14 30 39.449.4909-0.3867G49.488-0.387
e1/e244 GHz (I); 48.881.17126.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
19 23 43.9+14 30 39.449.4909-0.3867G49.488-0.387
e1/e244 GHz (I); 55.47.2126.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
2019 23 46.5+14 29 40.649.4815-0.4037G49.488-0.387
Met244 GHz (I); 52.370.6042.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
19 23 46.5+14 29 40.649.4815-0.4037G49.488-0.387
Met244 GHz (I); 54.040.6142.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
19 23 46.5+14 29 40.649.4815-0.4037G49.488-0.387
Met244 GHz (I); 56.670.3742.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
2319 23 45.2+14 29 45.549.4802-0.3984G49.488-0.387
Met344 GHz (I); 53.951.229.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
19 23 45.2+14 29 45.549.4802-0.3984G49.488-0.387
Met344 GHz (I); 56.630.4629.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
2519 23 43.9+14 29 25.449.4728-0.3965G49.488-0.387
Met144 GHz (I); 56.01.116.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
2618 53 18.6+01 14 57.734.25720.1532G34.257+0.153
44 GHz (I); 56.41.036.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFR_MIXEDHAS90
18 53 18.6+01 14 57.734.25720.1532G34.257+0.153
44 GHz (I); 58.261.336.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFR_MIXEDHAS90
2817 47 20.4-28 23 7.30.6667-0.0363G0.6667-0.0344
44 GHz (I); 6320390.00AVE0250+H2O +CH3OH I +CH3OH II -OH SFRHAS90
17 47 20.4-28 23 7.30.6667-0.0363G0.6667-0.0344
44 GHz (I); 6320390.00AVE0250+H2O +CH3OH I +CH3OH II -OH SFRHAS90
3019 23 43.2+14 31 34.449.5031-0.3772G49.488-0.387
Met444 GHz (I); 64.42.648.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
3119 23 38.2+14 30 0549.4716-0.3709G49.488-0.387
Met544 GHz (I); 66.720.2914.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
3206 41 9.7+09 29 34.9203.31552.0549G203.316+2.055
44 GHz (I); 7.240.21107.00AVE0250+H2O +CH3OH I +CH3OH II SFR_MIXEDHAS90
06 41 9.7+09 29 34.9203.31552.0549G203.316+2.055
44 GHz (I); 7.520.46107.00AVE0250+H2O +CH3OH I +CH3OH II SFR_MIXEDHAS90
3420 38 36.8+42 37 59.581.87750.7838G81.876+0.782
(N)44 GHz (I); 8.920.3223.10AVE0250+H2O +CH3OH I +CH3OH II +OH SFR_MIXEDHAS90
3518 47 47-01 54 35.130.8157-0.0580G30.817-0.057
44 GHz (I); 95.151.4228.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
18 47 47-01 54 35.130.8157-0.0580G30.817-0.057
44 GHz (I); 96.810.9228.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
18 47 47-01 54 35.130.8157-0.0580G30.817-0.057
44 GHz (I); 99.193228.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
18 47 47-01 54 35.130.8157-0.0580G30.817-0.057
44 GHz (I); 102.43228.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
3905 40 53.3+35 41 48.8173.71882.6980G173.719+2.698
44 GHz (I); -16.380.7461.40AVE0250+H2O +CH3OH I +CH3OH II -OH SFR_MIXEDHAS90
05 40 53.3+35 41 48.8173.71882.6980G173.719+2.698
44 GHz (I); -170.1761.40AVE0250+H2O +CH3OH I +CH3OH II -OH SFR_MIXEDHAS90
4120 38 54.6+42 19 23.581.66440.5521G81.711+0.563
West44 GHz (I); -2.470.35132.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
20 38 54.6+42 19 23.581.66440.5521G81.711+0.563
West44 GHz (I); -1.951.6132.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
20 38 54.6+42 19 23.581.66440.5521G81.711+0.563
West44 GHz (I); -1.50.22132.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
4420 39 00+42 19 27.881.67550.5396G81.711+0.563
44 GHz (I); -3.82.624.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
4520 39 0.7+42 22 50.881.72160.5722G81.711+0.563
44 GHz (I); -4.81.9329.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
20 39 0.7+42 22 50.881.72160.5722G81.711+0.563
44 GHz (I); -1.12.6329.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
20 39 0.7+42 22 50.881.72160.5722G81.711+0.563
44 GHz (I); 0.360.66329.00AVE0250+H2O +CH3OH I +CH3OH II +OH -SiO SFRHAS90
4802 27 4.7+61 52 25.5133.94881.0651G133.949+1.064
44 GHz (I); -46.490.84.20AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
4923 13 44.8+61 26 50.7111.53300.7567G111.542+0.769
44 GHz (I); -55.65.263.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
5017 20 53.3-35 47 1.5351.41680.6453G351.417+0.645
44 GHz (I); -6.15.4150.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFR_MIXEDHAS90
5122 19 18.3+63 18 48.3106.79725.3122G106.797+5.312
44 GHz (I); -8.220.712.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFRHAS90
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Non-detection table from Haschick et al. (1990)

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ID Obs. RA Obs. Dec l b Group id Line ∫F dv List Beam Detection Class Ref.
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (Jy*km/s) (arcsec) Yes/No
118 10 28.5-19 55 48.710.6233-0.3830G10.623-0.383
44 GHz (I); 88.00AVE0250+H2O +CH3OH I +CH3OH II +OH SFR_MIXEDHAS90
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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 HAS90

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

  • Distribution of sources from HAS90 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

    Download 2MASS K FITS