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FOR90 - Molecules and masers near compact H II regions

Short title: Forster et al. (1990)
Authors: Forster, J. R. Caswell, J. L. Okumura, S. K. Hasegawa, T. Ishiguro, M.
Journal: Astronomy and Astrophysics (ISSN 0004-6361), vol. 231, no. 2, May 1990, p. 473-480.
Bibcode: 1990A&A...231..473F

PDF: FOR90.pdf

Detection table from Forster et al. (1990)

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ID Obs. RA Obs. Dec l b Group id Line Vpeak FWHM List Beam Detection Ref.
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (km/s) (km/s) (arcsec) Yes/No
117 50 14.4-28 54 29.60.5465-0.8511G0.543-0.855
44 GHz (I)
17.26.1AVE0240+CH3OH I +CH3OH II +OH FOR90
218 06 19.1-21 37 31.98.6694-0.3561G8.669-0.357
44 GHz (I)
35.23.0AVE0240+H2O +CH3OH I +CH3OH II +OH FOR90
318 00 30.3-24 04 1.55.8850-0.3921G5.885-0.392
44 GHz (I)
8.31.2AVE0240+H2O +CH3OH I +CH3OH II +OH FOR90
417 26 42.3-36 09 16.4351.7744-0.5355G351.775-0.537
44 GHz (I)
-2.41.4AVE0240+H2O +CH3OH I +CH3OH II +OH FOR90
502 27 3.9+61 52 24.6133.94751.0642G133.948+1.064
44 GHz (I)
-47.74.8AVE0240+H2O +CH3OH I +CH3OH II +OH FOR90
618 53 18.5+01 14 58.734.25730.1537G34.257+0.153
44 GHz (I)
57.14.7AVE0240+H2O +CH3OH I +CH3OH II +OH FOR90
723 13 45.3+61 28 10.7111.54210.7770G111.542+0.766
44 GHz (I)
-57.62.1AVE0240+H2O +CH3OH I +CH3OH II +OH FOR90
818 10 28.6-19 55 50.710.6230-0.3836G10.623-0.383
44 GHz (I)
-7.32.6AVE0240+H2O +CH3OH I +CH3OH II +OH FOR90
917 20 53.4-35 47 1.5351.41700.6450G351.417+0.645
44 GHz (I)
-7.64.6AVE0240+H2O +CH3OH I +CH3OH II +OH FOR90
1017 25 25.3-36 12 44351.5817-0.3530G351.581-0.353
44 GHz (I)
-95.67.5AVE0240+H2O +CH3OH I +CH3OH II +OH FOR90
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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 FOR90

    Tip: Use "Box select" or "Lasso select" to display velocity-selected sources in Aladin all-sky view

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

  • Distribution of sources from FOR90 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